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GitHub - ankrh/MCmatlab: Numerical simulation tool for Monte Carlo propagation of light in turbid media

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nav&quot;,&quot;action&quot;:&quot;click to Sign in&quot;,&quot;label&quot;:&quot;ref_page:Marketing;ref_cta:Sign in;ref_loc:Header&quot;}" > Sign in </a> </div> </div> <div class="HeaderMenu js-header-menu height-fit position-lg-relative d-lg-flex flex-column flex-auto top-0"> <div class="HeaderMenu-wrapper d-flex flex-column flex-self-start flex-lg-row flex-auto rounded rounded-lg-0"> <nav class="HeaderMenu-nav" aria-label="Global"> <ul class="d-lg-flex list-style-none"> <li class="HeaderMenu-item position-relative flex-wrap flex-justify-between flex-items-center d-block d-lg-flex flex-lg-nowrap flex-lg-items-center js-details-container js-header-menu-item"> <button type="button" class="HeaderMenu-link border-0 width-full width-lg-auto px-0 px-lg-2 py-lg-2 no-wrap d-flex flex-items-center flex-justify-between js-details-target" aria-expanded="false"> Product <svg opacity="0.5" aria-hidden="true" height="16" viewBox="0 0 16 16" version="1.1" width="16" data-view-component="true" class="octicon octicon-chevron-down HeaderMenu-icon ml-1"> <path d="M12.78 5.22a.749.749 0 0 1 0 1.06l-4.25 4.25a.749.749 0 0 1-1.06 0L3.22 6.28a.749.749 0 1 1 1.06-1.06L8 8.939l3.72-3.719a.749.749 0 0 1 1.06 0Z"></path> </svg> </button> <div class="HeaderMenu-dropdown dropdown-menu rounded m-0 p-0 pt-2 pt-lg-4 position-relative position-lg-absolute left-0 left-lg-n3 pb-2 pb-lg-4 d-lg-flex flex-wrap dropdown-menu-wide"> <div class="HeaderMenu-column px-lg-4 border-lg-right mb-4 mb-lg-0 pr-lg-7"> <div class="border-bottom pb-3 pb-lg-0 border-lg-bottom-0"> <ul class="list-style-none f5" > <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary d-flex flex-items-center Link--has-description pb-lg-3" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;github_copilot&quot;,&quot;context&quot;:&quot;product&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;github_copilot_link_product_navbar&quot;}" href="https://github.com/features/copilot"> <svg aria-hidden="true" height="24" viewBox="0 0 24 24" version="1.1" width="24" data-view-component="true" class="octicon octicon-copilot color-fg-subtle mr-3"> <path d="M23.922 16.992c-.861 1.495-5.859 5.023-11.922 5.023-6.063 0-11.061-3.528-11.922-5.023A.641.641 0 0 1 0 16.736v-2.869a.841.841 0 0 1 .053-.22c.372-.935 1.347-2.292 2.605-2.656.167-.429.414-1.055.644-1.517a10.195 10.195 0 0 1-.052-1.086c0-1.331.282-2.499 1.132-3.368.397-.406.89-.717 1.474-.952 1.399-1.136 3.392-2.093 6.122-2.093 2.731 0 4.767.957 6.166 2.093.584.235 1.077.546 1.474.952.85.869 1.132 2.037 1.132 3.368 0 .368-.014.733-.052 1.086.23.462.477 1.088.644 1.517 1.258.364 2.233 1.721 2.605 2.656a.832.832 0 0 1 .053.22v2.869a.641.641 0 0 1-.078.256ZM12.172 11h-.344a4.323 4.323 0 0 1-.355.508C10.703 12.455 9.555 13 7.965 13c-1.725 0-2.989-.359-3.782-1.259a2.005 2.005 0 0 1-.085-.104L4 11.741v6.585c1.435.779 4.514 2.179 8 2.179 3.486 0 6.565-1.4 8-2.179v-6.585l-.098-.104s-.033.045-.085.104c-.793.9-2.057 1.259-3.782 1.259-1.59 0-2.738-.545-3.508-1.492a4.323 4.323 0 0 1-.355-.508h-.016.016Zm.641-2.935c.136 1.057.403 1.913.878 2.497.442.544 1.134.938 2.344.938 1.573 0 2.292-.337 2.657-.751.384-.435.558-1.15.558-2.361 0-1.14-.243-1.847-.705-2.319-.477-.488-1.319-.862-2.824-1.025-1.487-.161-2.192.138-2.533.529-.269.307-.437.808-.438 1.578v.021c0 .265.021.562.063.893Zm-1.626 0c.042-.331.063-.628.063-.894v-.02c-.001-.77-.169-1.271-.438-1.578-.341-.391-1.046-.69-2.533-.529-1.505.163-2.347.537-2.824 1.025-.462.472-.705 1.179-.705 2.319 0 1.211.175 1.926.558 2.361.365.414 1.084.751 2.657.751 1.21 0 1.902-.394 2.344-.938.475-.584.742-1.44.878-2.497Z"></path><path d="M14.5 14.25a1 1 0 0 1 1 1v2a1 1 0 0 1-2 0v-2a1 1 0 0 1 1-1Zm-5 0a1 1 0 0 1 1 1v2a1 1 0 0 1-2 0v-2a1 1 0 0 1 1-1Z"></path> </svg> <div> <div class="color-fg-default h4">GitHub Copilot</div> Write better code with AI </div> </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary d-flex flex-items-center Link--has-description pb-lg-3" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;github_advanced_security&quot;,&quot;context&quot;:&quot;product&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;github_advanced_security_link_product_navbar&quot;}" href="https://github.com/security/advanced-security"> <svg aria-hidden="true" height="24" viewBox="0 0 24 24" version="1.1" width="24" data-view-component="true" class="octicon octicon-shield-check color-fg-subtle mr-3"> <path d="M16.53 9.78a.75.75 0 0 0-1.06-1.06L11 13.19l-1.97-1.97a.75.75 0 0 0-1.06 1.06l2.5 2.5a.75.75 0 0 0 1.06 0l5-5Z"></path><path d="m12.54.637 8.25 2.675A1.75 1.75 0 0 1 22 4.976V10c0 6.19-3.771 10.704-9.401 12.83a1.704 1.704 0 0 1-1.198 0C5.77 20.705 2 16.19 2 10V4.976c0-.758.489-1.43 1.21-1.664L11.46.637a1.748 1.748 0 0 1 1.08 0Zm-.617 1.426-8.25 2.676a.249.249 0 0 0-.173.237V10c0 5.46 3.28 9.483 8.43 11.426a.199.199 0 0 0 .14 0C17.22 19.483 20.5 15.461 20.5 10V4.976a.25.25 0 0 0-.173-.237l-8.25-2.676a.253.253 0 0 0-.154 0Z"></path> </svg> <div> <div class="color-fg-default h4">GitHub Advanced Security</div> Find and fix vulnerabilities </div> </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary d-flex flex-items-center Link--has-description pb-lg-3" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;actions&quot;,&quot;context&quot;:&quot;product&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;actions_link_product_navbar&quot;}" href="https://github.com/features/actions"> <svg aria-hidden="true" height="24" viewBox="0 0 24 24" version="1.1" width="24" data-view-component="true" class="octicon octicon-workflow color-fg-subtle mr-3"> <path d="M1 3a2 2 0 0 1 2-2h6.5a2 2 0 0 1 2 2v6.5a2 2 0 0 1-2 2H7v4.063C7 16.355 7.644 17 8.438 17H12.5v-2.5a2 2 0 0 1 2-2H21a2 2 0 0 1 2 2V21a2 2 0 0 1-2 2h-6.5a2 2 0 0 1-2-2v-2.5H8.437A2.939 2.939 0 0 1 5.5 15.562V11.5H3a2 2 0 0 1-2-2Zm2-.5a.5.5 0 0 0-.5.5v6.5a.5.5 0 0 0 .5.5h6.5a.5.5 0 0 0 .5-.5V3a.5.5 0 0 0-.5-.5ZM14.5 14a.5.5 0 0 0-.5.5V21a.5.5 0 0 0 .5.5H21a.5.5 0 0 0 .5-.5v-6.5a.5.5 0 0 0-.5-.5Z"></path> </svg> <div> <div class="color-fg-default h4">Actions</div> Automate any workflow </div> </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary d-flex flex-items-center Link--has-description pb-lg-3" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;codespaces&quot;,&quot;context&quot;:&quot;product&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;codespaces_link_product_navbar&quot;}" href="https://github.com/features/codespaces"> <svg aria-hidden="true" height="24" viewBox="0 0 24 24" version="1.1" width="24" data-view-component="true" class="octicon octicon-codespaces color-fg-subtle mr-3"> <path d="M3.5 3.75C3.5 2.784 4.284 2 5.25 2h13.5c.966 0 1.75.784 1.75 1.75v7.5A1.75 1.75 0 0 1 18.75 13H5.25a1.75 1.75 0 0 1-1.75-1.75Zm-2 12c0-.966.784-1.75 1.75-1.75h17.5c.966 0 1.75.784 1.75 1.75v4a1.75 1.75 0 0 1-1.75 1.75H3.25a1.75 1.75 0 0 1-1.75-1.75ZM5.25 3.5a.25.25 0 0 0-.25.25v7.5c0 .138.112.25.25.25h13.5a.25.25 0 0 0 .25-.25v-7.5a.25.25 0 0 0-.25-.25Zm-2 12a.25.25 0 0 0-.25.25v4c0 .138.112.25.25.25h17.5a.25.25 0 0 0 .25-.25v-4a.25.25 0 0 0-.25-.25Z"></path><path d="M10 17.75a.75.75 0 0 1 .75-.75h6.5a.75.75 0 0 1 0 1.5h-6.5a.75.75 0 0 1-.75-.75Zm-4 0a.75.75 0 0 1 .75-.75h.5a.75.75 0 0 1 0 1.5h-.5a.75.75 0 0 1-.75-.75Z"></path> </svg> <div> <div class="color-fg-default h4">Codespaces</div> Instant dev environments </div> </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary d-flex flex-items-center Link--has-description pb-lg-3" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;issues&quot;,&quot;context&quot;:&quot;product&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;issues_link_product_navbar&quot;}" href="https://github.com/features/issues"> <svg aria-hidden="true" height="24" viewBox="0 0 24 24" version="1.1" width="24" data-view-component="true" class="octicon octicon-issue-opened color-fg-subtle mr-3"> <path d="M12 1c6.075 0 11 4.925 11 11s-4.925 11-11 11S1 18.075 1 12 5.925 1 12 1ZM2.5 12a9.5 9.5 0 0 0 9.5 9.5 9.5 9.5 0 0 0 9.5-9.5A9.5 9.5 0 0 0 12 2.5 9.5 9.5 0 0 0 2.5 12Zm9.5 2a2 2 0 1 1-.001-3.999A2 2 0 0 1 12 14Z"></path> </svg> <div> <div class="color-fg-default h4">Issues</div> Plan and track work </div> </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary d-flex flex-items-center Link--has-description pb-lg-3" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;code_review&quot;,&quot;context&quot;:&quot;product&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;code_review_link_product_navbar&quot;}" href="https://github.com/features/code-review"> <svg aria-hidden="true" height="24" viewBox="0 0 24 24" version="1.1" width="24" data-view-component="true" class="octicon octicon-code-review color-fg-subtle mr-3"> <path d="M10.3 6.74a.75.75 0 0 1-.04 1.06l-2.908 2.7 2.908 2.7a.75.75 0 1 1-1.02 1.1l-3.5-3.25a.75.75 0 0 1 0-1.1l3.5-3.25a.75.75 0 0 1 1.06.04Zm3.44 1.06a.75.75 0 1 1 1.02-1.1l3.5 3.25a.75.75 0 0 1 0 1.1l-3.5 3.25a.75.75 0 1 1-1.02-1.1l2.908-2.7-2.908-2.7Z"></path><path d="M1.5 4.25c0-.966.784-1.75 1.75-1.75h17.5c.966 0 1.75.784 1.75 1.75v12.5a1.75 1.75 0 0 1-1.75 1.75h-9.69l-3.573 3.573A1.458 1.458 0 0 1 5 21.043V18.5H3.25a1.75 1.75 0 0 1-1.75-1.75ZM3.25 4a.25.25 0 0 0-.25.25v12.5c0 .138.112.25.25.25h2.5a.75.75 0 0 1 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1.75 1ZM1.5 2.75v9.5c0 .138.112.25.25.25h2a.75.75 0 0 1 .75.75v2.19l2.72-2.72a.749.749 0 0 1 .53-.22h6.5a.25.25 0 0 0 .25-.25v-9.5a.25.25 0 0 0-.25-.25H1.75a.25.25 0 0 0-.25.25Z"></path><path d="M22.5 8.75a.25.25 0 0 0-.25-.25h-3.5a.75.75 0 0 1 0-1.5h3.5c.966 0 1.75.784 1.75 1.75v9.5A1.75 1.75 0 0 1 22.25 20H21v1.543a1.457 1.457 0 0 1-2.487 1.03L15.939 20H10.75A1.75 1.75 0 0 1 9 18.25v-1.465a.75.75 0 0 1 1.5 0v1.465c0 .138.112.25.25.25h5.5a.75.75 0 0 1 .53.22l2.72 2.72v-2.19a.75.75 0 0 1 .75-.75h2a.25.25 0 0 0 .25-.25v-9.5Z"></path> </svg> <div> <div class="color-fg-default h4">Discussions</div> Collaborate outside of code </div> </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary d-flex flex-items-center Link--has-description" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;code_search&quot;,&quot;context&quot;:&quot;product&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;code_search_link_product_navbar&quot;}" href="https://github.com/features/code-search"> <svg aria-hidden="true" height="24" viewBox="0 0 24 24" version="1.1" width="24" data-view-component="true" class="octicon octicon-code-square color-fg-subtle mr-3"> <path d="M10.3 8.24a.75.75 0 0 1-.04 1.06L7.352 12l2.908 2.7a.75.75 0 1 1-1.02 1.1l-3.5-3.25a.75.75 0 0 1 0-1.1l3.5-3.25a.75.75 0 0 1 1.06.04Zm3.44 1.06a.75.75 0 1 1 1.02-1.1l3.5 3.25a.75.75 0 0 1 0 1.1l-3.5 3.25a.75.75 0 1 1-1.02-1.1l2.908-2.7-2.908-2.7Z"></path><path d="M2 3.75C2 2.784 2.784 2 3.75 2h16.5c.966 0 1.75.784 1.75 1.75v16.5A1.75 1.75 0 0 1 20.25 22H3.75A1.75 1.75 0 0 1 2 20.25Zm1.75-.25a.25.25 0 0 0-.25.25v16.5c0 .138.112.25.25.25h16.5a.25.25 0 0 0 .25-.25V3.75a.25.25 0 0 0-.25-.25Z"></path> </svg> <div> <div class="color-fg-default h4">Code Search</div> Find more, search less </div> </a></li> </ul> </div> </div> <div class="HeaderMenu-column px-lg-4"> <div class="border-bottom pb-3 pb-lg-0 border-lg-bottom-0 border-bottom-0"> <span class="d-block h4 color-fg-default my-1" id="product-explore-heading">Explore</span> <ul class="list-style-none f5" aria-labelledby="product-explore-heading"> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;all_features&quot;,&quot;context&quot;:&quot;product&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;all_features_link_product_navbar&quot;}" href="https://github.com/features"> All features </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary Link--external" target="_blank" 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</li> <li class="HeaderMenu-item position-relative flex-wrap flex-justify-between flex-items-center d-block d-lg-flex flex-lg-nowrap flex-lg-items-center js-details-container js-header-menu-item"> <button type="button" class="HeaderMenu-link border-0 width-full width-lg-auto px-0 px-lg-2 py-lg-2 no-wrap d-flex flex-items-center flex-justify-between js-details-target" aria-expanded="false"> Solutions <svg opacity="0.5" aria-hidden="true" height="16" viewBox="0 0 16 16" version="1.1" width="16" data-view-component="true" class="octicon octicon-chevron-down HeaderMenu-icon ml-1"> <path d="M12.78 5.22a.749.749 0 0 1 0 1.06l-4.25 4.25a.749.749 0 0 1-1.06 0L3.22 6.28a.749.749 0 1 1 1.06-1.06L8 8.939l3.72-3.719a.749.749 0 0 1 1.06 0Z"></path> </svg> </button> <div class="HeaderMenu-dropdown dropdown-menu rounded m-0 p-0 pt-2 pt-lg-4 position-relative position-lg-absolute left-0 left-lg-n3 d-lg-flex flex-wrap dropdown-menu-wide"> <div class="HeaderMenu-column px-lg-4 border-lg-right mb-4 mb-lg-0 pr-lg-7"> <div class="border-bottom pb-3 pb-lg-0 border-lg-bottom-0 pb-lg-3 mb-3 mb-lg-0"> <span class="d-block h4 color-fg-default my-1" id="solutions-by-company-size-heading">By company size</span> <ul class="list-style-none f5" aria-labelledby="solutions-by-company-size-heading"> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;enterprises&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;enterprises_link_solutions_navbar&quot;}" href="https://github.com/enterprise"> Enterprises </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;small_and_medium_teams&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;small_and_medium_teams_link_solutions_navbar&quot;}" href="https://github.com/team"> Small and medium teams </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;startups&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;startups_link_solutions_navbar&quot;}" href="https://github.com/enterprise/startups"> Startups </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;nonprofits&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;nonprofits_link_solutions_navbar&quot;}" href="/solutions/industry/nonprofits"> Nonprofits </a></li> </ul> </div> <div class="border-bottom pb-3 pb-lg-0 border-lg-bottom-0"> <span class="d-block h4 color-fg-default my-1" id="solutions-by-use-case-heading">By use case</span> <ul class="list-style-none f5" aria-labelledby="solutions-by-use-case-heading"> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;devsecops&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;devsecops_link_solutions_navbar&quot;}" href="/solutions/use-case/devsecops"> DevSecOps </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;devops&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;devops_link_solutions_navbar&quot;}" href="/solutions/use-case/devops"> DevOps </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;ci_cd&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;ci_cd_link_solutions_navbar&quot;}" href="/solutions/use-case/ci-cd"> CI/CD </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;view_all_use_cases&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;view_all_use_cases_link_solutions_navbar&quot;}" href="/solutions/use-case"> View all use cases </a></li> </ul> </div> </div> <div class="HeaderMenu-column px-lg-4"> <div class="border-bottom pb-3 pb-lg-0 border-lg-bottom-0"> <span class="d-block h4 color-fg-default my-1" id="solutions-by-industry-heading">By industry</span> <ul class="list-style-none f5" aria-labelledby="solutions-by-industry-heading"> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;healthcare&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;healthcare_link_solutions_navbar&quot;}" href="/solutions/industry/healthcare"> Healthcare </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;financial_services&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;financial_services_link_solutions_navbar&quot;}" href="/solutions/industry/financial-services"> Financial services </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;manufacturing&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;manufacturing_link_solutions_navbar&quot;}" href="/solutions/industry/manufacturing"> Manufacturing </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;government&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;government_link_solutions_navbar&quot;}" href="/solutions/industry/government"> Government </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;view_all_industries&quot;,&quot;context&quot;:&quot;solutions&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;view_all_industries_link_solutions_navbar&quot;}" href="/solutions/industry"> View all industries </a></li> </ul> </div> </div> <div class="HeaderMenu-trailing-link rounded-bottom-2 flex-shrink-0 mt-lg-4 px-lg-4 py-4 py-lg-3 f5 text-semibold"> <a href="/solutions"> View all solutions <svg aria-hidden="true" height="16" viewBox="0 0 16 16" version="1.1" width="16" data-view-component="true" class="octicon octicon-chevron-right HeaderMenu-trailing-link-icon"> <path d="M6.22 3.22a.75.75 0 0 1 1.06 0l4.25 4.25a.75.75 0 0 1 0 1.06l-4.25 4.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042L9.94 8 6.22 4.28a.75.75 0 0 1 0-1.06Z"></path> </svg> </a> </div> </div> </li> <li class="HeaderMenu-item position-relative flex-wrap flex-justify-between flex-items-center d-block d-lg-flex flex-lg-nowrap flex-lg-items-center js-details-container js-header-menu-item"> <button type="button" class="HeaderMenu-link border-0 width-full width-lg-auto px-0 px-lg-2 py-lg-2 no-wrap d-flex flex-items-center flex-justify-between js-details-target" aria-expanded="false"> Resources <svg opacity="0.5" aria-hidden="true" height="16" viewBox="0 0 16 16" version="1.1" width="16" data-view-component="true" class="octicon octicon-chevron-down HeaderMenu-icon ml-1"> <path d="M12.78 5.22a.749.749 0 0 1 0 1.06l-4.25 4.25a.749.749 0 0 1-1.06 0L3.22 6.28a.749.749 0 1 1 1.06-1.06L8 8.939l3.72-3.719a.749.749 0 0 1 1.06 0Z"></path> </svg> </button> <div class="HeaderMenu-dropdown dropdown-menu rounded m-0 p-0 pt-2 pt-lg-4 position-relative position-lg-absolute left-0 left-lg-n3 pb-2 pb-lg-4 d-lg-flex flex-wrap dropdown-menu-wide"> <div class="HeaderMenu-column px-lg-4 border-lg-right mb-4 mb-lg-0 pr-lg-7"> <div class="border-bottom pb-3 pb-lg-0 border-lg-bottom-0"> <span class="d-block h4 color-fg-default my-1" id="resources-topics-heading">Topics</span> <ul class="list-style-none f5" aria-labelledby="resources-topics-heading"> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;ai&quot;,&quot;context&quot;:&quot;resources&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;ai_link_resources_navbar&quot;}" href="/resources/articles/ai"> AI </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;devops&quot;,&quot;context&quot;:&quot;resources&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;devops_link_resources_navbar&quot;}" href="/resources/articles/devops"> DevOps </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;security&quot;,&quot;context&quot;:&quot;resources&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;security_link_resources_navbar&quot;}" href="/resources/articles/security"> Security </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;software_development&quot;,&quot;context&quot;:&quot;resources&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;software_development_link_resources_navbar&quot;}" href="/resources/articles/software-development"> Software Development </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;view_all&quot;,&quot;context&quot;:&quot;resources&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;view_all_link_resources_navbar&quot;}" href="/resources/articles"> View all </a></li> </ul> </div> </div> <div class="HeaderMenu-column px-lg-4"> <div class="border-bottom pb-3 pb-lg-0 border-lg-bottom-0 border-bottom-0"> <span class="d-block h4 color-fg-default my-1" id="resources-explore-heading">Explore</span> <ul class="list-style-none f5" aria-labelledby="resources-explore-heading"> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary Link--external" target="_blank" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;learning_pathways&quot;,&quot;context&quot;:&quot;resources&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;learning_pathways_link_resources_navbar&quot;}" href="https://resources.github.com/learn/pathways"> Learning Pathways <svg aria-hidden="true" height="16" viewBox="0 0 16 16" version="1.1" width="16" data-view-component="true" class="octicon octicon-link-external HeaderMenu-external-icon color-fg-subtle"> <path d="M3.75 2h3.5a.75.75 0 0 1 0 1.5h-3.5a.25.25 0 0 0-.25.25v8.5c0 .138.112.25.25.25h8.5a.25.25 0 0 0 .25-.25v-3.5a.75.75 0 0 1 1.5 0v3.5A1.75 1.75 0 0 1 12.25 14h-8.5A1.75 1.75 0 0 1 2 12.25v-8.5C2 2.784 2.784 2 3.75 2Zm6.854-1h4.146a.25.25 0 0 1 .25.25v4.146a.25.25 0 0 1-.427.177L13.03 4.03 9.28 7.78a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042l3.75-3.75-1.543-1.543A.25.25 0 0 1 10.604 1Z"></path> </svg> </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary Link--external" target="_blank" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;events_amp_webinars&quot;,&quot;context&quot;:&quot;resources&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;events_amp_webinars_link_resources_navbar&quot;}" href="https://resources.github.com"> Events &amp; Webinars <svg aria-hidden="true" height="16" viewBox="0 0 16 16" version="1.1" width="16" data-view-component="true" class="octicon octicon-link-external HeaderMenu-external-icon color-fg-subtle"> <path d="M3.75 2h3.5a.75.75 0 0 1 0 1.5h-3.5a.25.25 0 0 0-.25.25v8.5c0 .138.112.25.25.25h8.5a.25.25 0 0 0 .25-.25v-3.5a.75.75 0 0 1 1.5 0v3.5A1.75 1.75 0 0 1 12.25 14h-8.5A1.75 1.75 0 0 1 2 12.25v-8.5C2 2.784 2.784 2 3.75 2Zm6.854-1h4.146a.25.25 0 0 1 .25.25v4.146a.25.25 0 0 1-.427.177L13.03 4.03 9.28 7.78a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042l3.75-3.75-1.543-1.543A.25.25 0 0 1 10.604 1Z"></path> </svg> </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" data-analytics-event="{&quot;location&quot;:&quot;navbar&quot;,&quot;action&quot;:&quot;ebooks_amp_whitepapers&quot;,&quot;context&quot;:&quot;resources&quot;,&quot;tag&quot;:&quot;link&quot;,&quot;label&quot;:&quot;ebooks_amp_whitepapers_link_resources_navbar&quot;}" href="https://github.com/resources/whitepapers"> Ebooks &amp; Whitepapers </a></li> <li> <a class="HeaderMenu-dropdown-link d-block no-underline position-relative py-2 Link--secondary" 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2.573A1.458 1.458 0 0 1 3 15.543V14H1.75A1.75 1.75 0 0 1 0 12.25v-9.5C0 1.784.784 1 1.75 1ZM1.5 2.75v9.5c0 .138.112.25.25.25h2a.75.75 0 0 1 .75.75v2.19l2.72-2.72a.749.749 0 0 1 .53-.22h6.5a.25.25 0 0 0 .25-.25v-9.5a.25.25 0 0 0-.25-.25H1.75a.25.25 0 0 0-.25.25Z"></path><path d="M22.5 8.75a.25.25 0 0 0-.25-.25h-3.5a.75.75 0 0 1 0-1.5h3.5c.966 0 1.75.784 1.75 1.75v9.5A1.75 1.75 0 0 1 22.25 20H21v1.543a1.457 1.457 0 0 1-2.487 1.03L15.939 20H10.75A1.75 1.75 0 0 1 9 18.25v-1.465a.75.75 0 0 1 1.5 0v1.465c0 .138.112.25.25.25h5.5a.75.75 0 0 1 .53.22l2.72 2.72v-2.19a.75.75 0 0 1 .75-.75h2a.25.25 0 0 0 .25-.25v-9.5Z"></path> </svg> <div> <div class="color-fg-default h4">Premium Support</div> Enterprise-grade 24/7 support </div> </a></li> </ul> </div> </div> </div> </li> <li class="HeaderMenu-item position-relative flex-wrap flex-justify-between flex-items-center d-block d-lg-flex flex-lg-nowrap flex-lg-items-center js-details-container js-header-menu-item"> <a class="HeaderMenu-link no-underline 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data-target="react-partial.embeddedData">{"props":{"initialPayload":{"allShortcutsEnabled":false,"path":"/","repo":{"id":435521074,"defaultBranch":"Release","name":"MCmatlab","ownerLogin":"ankrh","currentUserCanPush":false,"isFork":false,"isEmpty":false,"createdAt":"2021-12-06T14:08:40.000Z","ownerAvatar":"https://avatars.githubusercontent.com/u/95489031?v=4","public":true,"private":false,"isOrgOwned":false},"currentUser":null,"refInfo":{"name":"Release","listCacheKey":"v0:1742850544.0","canEdit":false,"refType":"branch","currentOid":"792f766fefa74459587db4aa728e4c2913bed8e7"},"tree":{"items":[{"name":"+MCmatlab","path":"+MCmatlab","contentType":"directory"},{"name":"helperfuncs","path":"helperfuncs","contentType":"directory"},{"name":".gitattributes","path":".gitattributes","contentType":"file"},{"name":".gitignore","path":".gitignore","contentType":"file"},{"name":"Example10_MediaPropertyParametricSweep.m","path":"Example10_MediaPropertyParametricSweep.m","contentType":"file"},{"name":"Example11_MultipleHeatSims.m","path":"Example11_MultipleHeatSims.m","contentType":"file"},{"name":"Example12_SaturableAbsorber.m","path":"Example12_SaturableAbsorber.m","contentType":"file"},{"name":"Example13_TdependentVHC.m","path":"Example13_TdependentVHC.m","contentType":"file"},{"name":"Example14_Thermochromism.m","path":"Example14_Thermochromism.m","contentType":"file"},{"name":"Example15_ThermallyInducedScattering.m","path":"Example15_ThermallyInducedScattering.m","contentType":"file"},{"name":"Example16_CUDAacceleration.m","path":"Example16_CUDAacceleration.m","contentType":"file"},{"name":"Example17_CurvedRefractionReflection.m","path":"Example17_CurvedRefractionReflection.m","contentType":"file"},{"name":"Example18_STLimport.m","path":"Example18_STLimport.m","contentType":"file"},{"name":"Example19_DepositionCriteria.m","path":"Example19_DepositionCriteria.m","contentType":"file"},{"name":"Example1_StandardTissue.m","path":"Example1_StandardTissue.m","contentType":"file"},{"name":"Example20_ReflectanceStatisticsAndCyclicBoundaries.m","path":"Example20_ReflectanceStatisticsAndCyclicBoundaries.m","contentType":"file"},{"name":"Example21_CustomPhaseFunctions.m","path":"Example21_CustomPhaseFunctions.m","contentType":"file"},{"name":"Example22_CombiningModelObjects.m","path":"Example22_CombiningModelObjects.m","contentType":"file"},{"name":"Example23_BroadbandMonteCarlo.m","path":"Example23_BroadbandMonteCarlo.m","contentType":"file"},{"name":"Example24_AzFzReflectanceTransmittance.m","path":"Example24_AzFzReflectanceTransmittance.m","contentType":"file"},{"name":"Example25_DepositionCriteria2.m","path":"Example25_DepositionCriteria2.m","contentType":"file"},{"name":"Example26_DistributedSource.m","path":"Example26_DistributedSource.m","contentType":"file"},{"name":"Example2_BeamDefinitions.m","path":"Example2_BeamDefinitions.m","contentType":"file"},{"name":"Example3_RefractionReflection.m","path":"Example3_RefractionReflection.m","contentType":"file"},{"name":"Example4_BloodVessel.m","path":"Example4_BloodVessel.m","contentType":"file"},{"name":"Example5_FluorescenceAndImaging.m","path":"Example5_FluorescenceAndImaging.m","contentType":"file"},{"name":"Example6_TimeTagging.m","path":"Example6_TimeTagging.m","contentType":"file"},{"name":"Example7_FarField.m","path":"Example7_FarField.m","contentType":"file"},{"name":"Example8_CollectedFluenceRate.m","path":"Example8_CollectedFluenceRate.m","contentType":"file"},{"name":"Example9_GeometryParametricSweep.m","path":"Example9_GeometryParametricSweep.m","contentType":"file"},{"name":"LICENSE","path":"LICENSE","contentType":"file"},{"name":"README.md","path":"README.md","contentType":"file"},{"name":"Test1_AllFRTDependences.m","path":"Test1_AllFRTDependences.m","contentType":"file"},{"name":"sample.stl","path":"sample.stl","contentType":"file"},{"name":"version","path":"version","contentType":"file"}],"templateDirectorySuggestionUrl":null,"readme":null,"totalCount":35,"showBranchInfobar":false},"fileTree":null,"fileTreeProcessingTime":null,"foldersToFetch":[],"treeExpanded":false,"symbolsExpanded":false,"isOverview":true,"overview":{"banners":{"shouldRecommendReadme":false,"isPersonalRepo":false,"showUseActionBanner":false,"actionSlug":null,"actionId":null,"showProtectBranchBanner":false,"publishBannersInfo":{"dismissActionNoticePath":"/settings/dismiss-notice/publish_action_from_repo","releasePath":"/ankrh/MCmatlab/releases/new?marketplace=true","showPublishActionBanner":false},"interactionLimitBanner":null,"showInvitationBanner":false,"inviterName":null,"actionsMigrationBannerInfo":{"releaseTags":[],"showImmutableActionsMigrationBanner":false,"initialMigrationStatus":null}},"codeButton":{"contactPath":"/contact","isEnterprise":false,"local":{"protocolInfo":{"httpAvailable":true,"sshAvailable":null,"httpUrl":"https://github.com/ankrh/MCmatlab.git","showCloneWarning":null,"sshUrl":null,"sshCertificatesRequired":null,"sshCertificatesAvailable":null,"ghCliUrl":"gh repo clone ankrh/MCmatlab","defaultProtocol":"http","newSshKeyUrl":"/settings/ssh/new","setProtocolPath":"/users/set_protocol"},"platformInfo":{"cloneUrl":"https://desktop.github.com","showVisualStudioCloneButton":false,"visualStudioCloneUrl":"https://windows.github.com","showXcodeCloneButton":false,"xcodeCloneUrl":"xcode://clone?repo=https%3A%2F%2Fgithub.com%2Fankrh%2FMCmatlab","zipballUrl":"/ankrh/MCmatlab/archive/refs/heads/Release.zip"}},"newCodespacePath":"/codespaces/new?hide_repo_select=true\u0026repo=435521074"},"popovers":{"rename":null,"renamedParentRepo":null},"commitCount":"610","overviewFiles":[{"displayName":"README.md","repoName":"MCmatlab","refName":"Release","path":"README.md","preferredFileType":"readme","tabName":"README","richText":"\u003carticle class=\"markdown-body entry-content container-lg\" itemprop=\"text\"\u003e\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch1 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eReadme and User Manual for MCmatlab\u003c/h1\u003e\u003ca id=\"user-content-readme-and-user-manual-for-mcmatlab\" class=\"anchor\" aria-label=\"Permalink: Readme and User Manual for MCmatlab\" href=\"#readme-and-user-manual-for-mcmatlab\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch2 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eWhat is MCmatlab?\u003c/h2\u003e\u003ca id=\"user-content-what-is-mcmatlab\" class=\"anchor\" aria-label=\"Permalink: What is MCmatlab?\" href=\"#what-is-mcmatlab\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eMCmatlab is a Monte Carlo simulation for modeling light propagation in a 3D voxel space. Fluorescence can optionally be simulated after simulation of the excitation light. Included is also a finite element simulation for temperature increase and heat diffusion in the same voxel space.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003ePrimarily targeted for tissue optics, but can be used in any environment with turbid media in which the wave nature of light (interference phenomena) is negligible and a ray-tracing model is appropriate.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003eYou can find the latest version of MCmatlab on \u003ca href=\"https://github.com/ankrh/MCmatlab\"\u003ehttps://github.com/ankrh/MCmatlab\u003c/a\u003e. You can also use MCmatlab directly in MATLAB online by clicking the button below. If you publish results obtained with this software, we would be thankful if you cited its accompanying article: doi:10.1117/1.JBO.23.12.121622\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ca href=\"https://matlab.mathworks.com/open/github/v1?repo=ankrh/MCmatlab\u0026amp;file=Example1_StandardTissue.m\" rel=\"nofollow\"\u003e\u003cimg src=\"https://camo.githubusercontent.com/2f3855e7dfae2344a326fab483b2599adfb2151c0630878b1deda2433bc5a8d4/68747470733a2f2f7777772e6d617468776f726b732e636f6d2f696d616765732f726573706f6e736976652f676c6f62616c2f6f70656e2d696e2d6d61746c61622d6f6e6c696e652e737667\" alt=\"Open in MATLAB Online\" data-canonical-src=\"https://www.mathworks.com/images/responsive/global/open-in-matlab-online.svg\" style=\"max-width: 100%;\"\u003e\u003c/a\u003e\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch2 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eLicense\u003c/h2\u003e\u003ca id=\"user-content-license\" class=\"anchor\" aria-label=\"Permalink: License\" href=\"#license\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eThis program is free software: you can redistribute it and/or modify\nit under the terms of the GNU General Public License as published by\nthe Free Software Foundation, either version 3 of the License, or\n(at your option) any later version.\nThis program is distributed in the hope that it will be useful,\nbut WITHOUT ANY WARRANTY; without even the implied warranty of\nMERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the\nGNU General Public License for more details.\nYou should have received a copy of the GNU General Public License\nalong with this program. If not, see \u003ca href=\"https://www.gnu.org/licenses/\" rel=\"nofollow\"\u003ehttps://www.gnu.org/licenses/\u003c/a\u003e.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch2 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eHow do I get set up?\u003c/h2\u003e\u003ca id=\"user-content-how-do-i-get-set-up\" class=\"anchor\" aria-label=\"Permalink: How do I get set up?\" href=\"#how-do-i-get-set-up\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eRequirements\u003c/h3\u003e\u003ca id=\"user-content-requirements\" class=\"anchor\" aria-label=\"Permalink: Requirements\" href=\"#requirements\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eWindows 7, macOS 10.12 (Sierra) or newer or Linux\u003c/li\u003e\n\u003cli\u003eMATLAB R2018a or newer (only the intel-versions of MATLAB are supported)\u003c/li\u003e\n\u003cli\u003e(For GPU accelerated computation) A Windows PC with a CUDA-enabled graphics card and the MATLAB Parallel Computing Toolbox\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eHelper files\u003c/h3\u003e\u003ca id=\"user-content-helper-files\" class=\"anchor\" aria-label=\"Permalink: Helper files\" href=\"#helper-files\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eAll the helper functions needed for running MCmatlab are located in the folder (MATLAB package) \"+MCmatlab\", and its parent folder therefore has to be on your MATLAB path when trying to run any MCmatlab model files. You will not need to modify any of the contained files. We recommend keeping the model files in a folder together with the \"+MCmatlab\" folder, such that you don't need to manually add the parent folder of \"+MCmatlab\" to your MATLAB path.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch2 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eHow do I use MCmatlab?\u003c/h2\u003e\u003ca id=\"user-content-how-do-i-use-mcmatlab\" class=\"anchor\" aria-label=\"Permalink: How do I use MCmatlab?\" href=\"#how-do-i-use-mcmatlab\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eCompilation\u003c/h3\u003e\u003ca id=\"user-content-compilation\" class=\"anchor\" aria-label=\"Permalink: Compilation\" href=\"#compilation\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eThe folders include all the executables necessary, so you don't need to compile anything. If, however, you want to change the routine in either the MCmatlab.c source code or the finiteElementHeatPropagator.c source code (both located in the folder \"+MCmatlab/src\"), you will need to recompile the respective mex-files. Check out those two source-files on how to do so. The source code is written in such a way that it can be compiled as either C or C++ code using either GCC, MSVC, clang or as CUDA source code using NVCC.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eModel files\u003c/h3\u003e\u003ca id=\"user-content-model-files\" class=\"anchor\" aria-label=\"Permalink: Model files\" href=\"#model-files\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eIn MCmatlab, you set up your model in a single m-file called \"Model File\". You can find some examples of Model Files to get you started in the parent folder of \"+MCmatlab\". A complete list of parameters that can be set is provided below.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eModel object\u003c/h3\u003e\u003ca id=\"user-content-model-object\" class=\"anchor\" aria-label=\"Permalink: Model object\" href=\"#model-object\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eA \"Model Object\" stores all the parameters for a single Monte Carlo simulation: a single geometry and a single type of lightsource, together with all the results from the Monte Carlo (and optional heat transfer) simulation. The Model Object is an instance of the class MCmatlab.model, i.e., it's of the class \"model\" in the MATLAB-package \"MCmatlab\". One Model File can, if desired, generate multiple Model Objects with a different geometry and/or lightsource each.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003eModel Objects can be saved to and loaded from a standard binary MATLAB MAT-file like any other MATLAB variable. When loading a Model Object from a MATLAB MAT-file, the parent folder of \"+MCmatlab\" needs to be on your MATLAB path: prior to loading the Model Object, either navigate to the parent folder of \"+MCmatlab\" in the \"Current Folder\" view of MATLAB, or use the command \"addpath\" to add the parent folder of \"+MCmatlab\" to your path.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eMATLAB function definitions\u003c/h3\u003e\u003ca id=\"user-content-matlab-function-definitions\" class=\"anchor\" aria-label=\"Permalink: MATLAB function definitions\" href=\"#matlab-function-definitions\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eMCmatlab makes extensive use of user-defined functions, passed into the simulation in the form of function handles. For more information, see \u003ccode\u003ehttps://www.mathworks.com/help/matlab/matlab_prog/creating-a-function-handle.html\u003c/code\u003e. Inside other functions, nested functions can be defined anywhere, but in the main model file script, MATLAB requires that all functions are defined at the end of the m file.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eMedia properties\u003c/h3\u003e\u003ca id=\"user-content-media-properties\" class=\"anchor\" aria-label=\"Permalink: Media properties\" href=\"#media-properties\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eThe optical properties of all media are defined in a function at the end of the model file. The examples contain some media you can modify or copy-paste to your own model file, or you define your own media from scratch in your own models. All media properties functions must start with this line: \u003ccode\u003emediaProperties = MCmatlab.mediumProperties;\u003c/code\u003e in order to initialize the \u003ccode\u003emediaProperties\u003c/code\u003e variable as an array of \u003ccode\u003emediumProperties\u003c/code\u003e objects. Make sure that each media in a single model file has its distinct \"j\"-number, as this is the number you will refer to when building your model in the geometry function (see below).\u003c/p\u003e\n\u003cp dir=\"auto\"\u003eEach medium can be specified with up to 13 properties. Many of these may be specified either as a scalar or as function handles that can take wavelength, fluence rate (FR), temperature (T) and fractional damage (FD) as input:\u003c/p\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003e\u003ccode\u003ename\u003c/code\u003e - A char array containing the name of the medium, used for the visualization.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003emua\u003c/code\u003e - The absorption coefficient in units of 1/cm. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003emus\u003c/code\u003e - The scattering coefficient in units of 1/cm. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003eg\u003c/code\u003e - The scattering anisotropy (the mean cosine to the scattering angle), to be used in the Henyey-Greenstein phase function. It has no units. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003ecustomPhaseFunc\u003c/code\u003e - An alternative to specifying \u003ccode\u003eg\u003c/code\u003e. If specified, this must be a function handle that takes wavelength and polar scattering angle as inputs and yields the scattering phase function as output. This function does not need to be normalized.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003en\u003c/code\u003e - The refractive index. May be (a) scalar or (b) a function handle taking wavelength as input.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003eQY\u003c/code\u003e - The quantum yield of fluorescence, that is, photons of fluorescence emitted relative to excitation photons absorbed. It has no units. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003eES\u003c/code\u003e - The emission spectrum of the fluorescence emission, if any. Doesn't need to be normalized. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003eVHC\u003c/code\u003e - The volumetric heat capacity of the medium in units of J/(cm^3 K). May be (a) scalar or (b) a function handle taking T and FD as inputs.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003eTC\u003c/code\u003e - The thermal conductivity of the medium in units of W/(cm K). May be (a) scalar or (b) a function handle taking T and FD as inputs.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003eE\u003c/code\u003e - The Arrhenius activation energy in units of J/mol. Must be scalar.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003eA\u003c/code\u003e - The Arrhenius pre-exponential factor in units of 1/s. Must be scalar.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003enBins\u003c/code\u003e - The number of bins (sub-media) to split the medium into in case of media that have properties that depend on fluence rate (FR), temperature (T) or fractional damage (FD). Must be scalar.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cp dir=\"auto\"\u003eFor Monte Carlo simulations, \u003ccode\u003ename\u003c/code\u003e, \u003ccode\u003emua\u003c/code\u003e, \u003ccode\u003emus\u003c/code\u003e and either \u003ccode\u003eg\u003c/code\u003e or \u003ccode\u003ecustomPhaseFunc\u003c/code\u003e need be specified for all media.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003eFor fluorescence Monte Carlo simulations, the \u003ccode\u003eQY\u003c/code\u003e and \u003ccode\u003eES\u003c/code\u003e properties must additionally be specified for those media that fluoresce.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003eFor heat simulations, \u003ccode\u003eVHC\u003c/code\u003e and \u003ccode\u003eTC\u003c/code\u003e must be specified for all media.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003eFor heat simulations with calculation of tissue damage, \u003ccode\u003eE\u003c/code\u003e and \u003ccode\u003eA\u003c/code\u003e must be specified for those media that can be damaged.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eBuilding the model\u003c/h3\u003e\u003ca id=\"user-content-building-the-model\" class=\"anchor\" aria-label=\"Permalink: Building the model\" href=\"#building-the-model\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eYou build each model in a separate m-file. Each model requires the first two and optionally more of the following steps:\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e1. Build geometry\u003c/h4\u003e\u003ca id=\"user-content-1-build-geometry\" class=\"anchor\" aria-label=\"Permalink: 1. Build geometry\" href=\"#1-build-geometry\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eModify or add to \"mediaPropertiesFunc\" at the end of the model file to include the definitions of the media you're interested in. You may optionally include thermal and/or fluorescence properties.\u003c/li\u003e\n\u003cli\u003eIn your model file, specify the side lengths Lx, Ly, Lz of your model cuboid and the resolutions Nx, Ny, Nz.\u003c/li\u003e\n\u003cli\u003eThe \"GeomFunc\" you define at the end of the model file simply returns a 3D array containing the media definition for each voxel in the model cuboid. The media are referred to by a number, corresponding to the \"j\" defined in \"mediaPropertiesFunc\" at the end of the model file.\u003c/li\u003e\n\u003cli\u003eYou may optionally import your geometry from STL files as shown in example 18.\u003c/li\u003e\n\u003cli\u003eAfter this step, when calling \"plot(model,'G')\", you will be shown a figure with the geometry you defined.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e2. Calculate light distribution\u003c/h4\u003e\u003ca id=\"user-content-2-calculate-light-distribution\" class=\"anchor\" aria-label=\"Permalink: 2. Calculate light distribution\" href=\"#2-calculate-light-distribution\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eThe section \"%% Monte Carlo simulation\" in the model file contains the definitions for the Monte Carlo simulation.\u003c/li\u003e\n\u003cli\u003eAfter this step, when calling \"plot(model,'MC')\", you will be shown various figures; one with an overview of the optical properties, one with the absorbed light in the cuboid, one with the normalized fluence rate (NFR, roughly equivalent to normalized intensity or irradiance), and one showing the fluence rate at the cuboid boundaries (taking into account only the \u003cem\u003eexiting\u003c/em\u003e photon packages, not the incident beam). The last figure will only be shown if some of your cuboid boundaries are \"escaping\" boundaries, i.e., boundary type 1 (all boundaries are escaping boundaries) or 2 (only the top is an escaping boundary).\u003c/li\u003e\n\u003cli\u003e(Optional) If you set \"model.MC.nExamplePaths\" to an integer \u0026gt; 0, you will also be shown a plot with the paths of the number of photons you requested.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e3. (Optional) Include Fresnel reflection and refraction\u003c/h4\u003e\u003ca id=\"user-content-3-optional-include-fresnel-reflection-and-refraction\" class=\"anchor\" aria-label=\"Permalink: 3. (Optional) Include Fresnel reflection and refraction\" href=\"#3-optional-include-fresnel-reflection-and-refraction\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eCheck out \"Example3_RefractionReflection.m\" and \"Example17_CurvedRefractionReflection.m\" on how to implement changing refractive indices in your model.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e4. (Optional) Calculate fluorescence light distribution\u003c/h4\u003e\u003ca id=\"user-content-4-optional-calculate-fluorescence-light-distribution\" class=\"anchor\" aria-label=\"Permalink: 4. (Optional) Calculate fluorescence light distribution\" href=\"#4-optional-calculate-fluorescence-light-distribution\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eThe section \"%% Fluorescence Monte Carlo\" contains the parameters for a fluorescence simulation, to be run after the distribution of excitation light has been calculated.\u003c/li\u003e\n\u003cli\u003eTo be able to run this step, your geometry definitions needs to include the fluorescence wavelength, \"model.FMC.wavelength\". Additionally, at least one of your media should be defined fluorescent, by defining its quantum yield \u003ccode\u003eQY\u003c/code\u003e in \"mediaPropertiesFunc\" at the end of your model file.\u003c/li\u003e\n\u003cli\u003eAfter this step, when calling \"plot(model,'FMC')\", you will be shown the fluorescence emitter distribution, the fluorescent light fluence rate, the absorption within the cuboid, and the fluorescent light fluence rate at the cuboid boundaries.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e5. (Optional) Simulate heat distribution\u003c/h4\u003e\u003ca id=\"user-content-5-optional-simulate-heat-distribution\" class=\"anchor\" aria-label=\"Permalink: 5. (Optional) Simulate heat distribution\" href=\"#5-optional-simulate-heat-distribution\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eIn the \"%% Heat simulation\" section, you put the parameters for simulation of the temperature distribution, to be run after the Monte Carlo step(s)\u003c/li\u003e\n\u003cli\u003eTo simulate the heat diffusion, all media involved in the simulation must have the thermal properties volumetric heat capacity (VHC) and thermal conductivity (TC) defined in \"mediaPropertiesFunc\" at the end of your model file.\u003c/li\u003e\n\u003cli\u003eIf you want to model chemical changes such as tissue damage, the media that might undergo such change need to additionally have the Arrhenius activation energy (E) and the Arrhenius pre-exponential factor (A) defined.\u003c/li\u003e\n\u003cli\u003eDuring the heat simulation, you will see an illustration of the temperature in your modelled cuboid.\u003c/li\u003e\n\u003cli\u003eAfter this step, when calling \"plot(model,'HS')\", you will be shown various figures with the position of virtual temperature sensors in the cuboid, the temperature evolution at these positions, and whether there was some chemical change (based on the Arrhenius integral) in your cuboid.\u003c/li\u003e\n\u003cli\u003eYou can run multiple heat simulations defining different successive pulse trains as shown in \"Example11_MultipleHeatSims.m\"\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e6. (Optional) Imaging: Model the intensity distribution received by a detector/light collector\u003c/h4\u003e\u003ca id=\"user-content-6-optional-imaging-model-the-intensity-distribution-received-by-a-detectorlight-collector\" class=\"anchor\" aria-label=\"Permalink: 6. (Optional) Imaging: Model the intensity distribution received by a detector/light collector\" href=\"#6-optional-imaging-model-the-intensity-distribution-received-by-a-detectorlight-collector\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eInclude a light collector for the incident light Monte Carlo, the fluorescence Monte Carlo, or for both. The light collector can either be a pixel array detector or a single pixel detector (such as a fibre). You can also optionally make your detector time-resolved.\u003c/li\u003e\n\u003cli\u003eAfter running and calling either \"plot(model,'MC')\" or \"plot(model,'FMC')\", you will see an illustration of the geometry of your imaging system and the image of the scattered and/or fluorescence light.\u003c/li\u003e\n\u003cli\u003eYou can also choose to show the light impinging on the light collector in a time-resolved manner. Check out \"Example6_TimeTagging.m\" on how to do so.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e7. (Optional) Calculate the far field angular distribution of light escaping the simulation volume\u003c/h4\u003e\u003ca id=\"user-content-7-optional-calculate-the-far-field-angular-distribution-of-light-escaping-the-simulation-volume\" class=\"anchor\" aria-label=\"Permalink: 7. (Optional) Calculate the far field angular distribution of light escaping the simulation volume\" href=\"#7-optional-calculate-the-far-field-angular-distribution-of-light-escaping-the-simulation-volume\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eSee \"Example7_FarField.m\". Note that the far field does not include \"killed\" photons, that is, photons that have exited at a boundary where the refractive index is different to 1, or photons that exit on boundaries that are not \"escaping\".\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e8. (Optional) Use deposition criteria to show the normalized fluence rate array of only those photons which end up on the detector\u003c/h4\u003e\u003ca id=\"user-content-8-optional-use-deposition-criteria-to-show-the-normalized-fluence-rate-array-of-only-those-photons-which-end-up-on-the-detector\" class=\"anchor\" aria-label=\"Permalink: 8. (Optional) Use deposition criteria to show the normalized fluence rate array of only those photons which end up on the detector\" href=\"#8-optional-use-deposition-criteria-to-show-the-normalized-fluence-rate-array-of-only-those-photons-which-end-up-on-the-detector\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eSee \"Example8_CollectedFluenceRate.m\".\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e9. (Optional) Programmatically assign values to the parameters\u003c/h4\u003e\u003ca id=\"user-content-9-optional-programmatically-assign-values-to-the-parameters\" class=\"anchor\" aria-label=\"Permalink: 9. (Optional) Programmatically assign values to the parameters\" href=\"#9-optional-programmatically-assign-values-to-the-parameters\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eSee \"Example9_GeometryParametricSweep.m\" and \"Example10_MediaPropertyParametricSweep.m\" on how to implement sweeps of the parameters.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e10. (Optional) Define fluence rate-, temperature- or fractional damage-dependent optical or thermal properties\u003c/h4\u003e\u003ca id=\"user-content-10-optional-define-fluence-rate--temperature--or-fractional-damage-dependent-optical-or-thermal-properties\" class=\"anchor\" aria-label=\"Permalink: 10. (Optional) Define fluence rate-, temperature- or fractional damage-dependent optical or thermal properties\" href=\"#10-optional-define-fluence-rate--temperature--or-fractional-damage-dependent-optical-or-thermal-properties\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eSee Examples 12-15.\u003c/li\u003e\n\u003cli\u003eBy specifying the optical or thermal properties as a string (technically a char array) defining the formula as a function of fluence rate (FR), temperature (T) or fractional damage (FD), MCmatlab will take the dependence into account with an iterative approach.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e11. (Optional) Enable CUDA GPU acceleration\u003c/h4\u003e\u003ca id=\"user-content-11-optional-enable-cuda-gpu-acceleration\" class=\"anchor\" aria-label=\"Permalink: 11. (Optional) Enable CUDA GPU acceleration\" href=\"#11-optional-enable-cuda-gpu-acceleration\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003eSee Example16_CUDAacceleration.m.\u003c/li\u003e\n\u003cli\u003eIf you have an Nvidia graphics card with compute capability at least 3.0, you can set useGPU = true to enable running on the GPU, greatly speeding up both the Monte Carlo and heat simulations.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eList and explanation of input parameters\u003c/h3\u003e\u003ca id=\"user-content-list-and-explanation-of-input-parameters\" class=\"anchor\" aria-label=\"Permalink: List and explanation of input parameters\" href=\"#list-and-explanation-of-input-parameters\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eIn the following we assume that the model object variable has been named \"model\". In principle, it could be given any name you want.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eGeometry parameters\u003c/h4\u003e\u003ca id=\"user-content-geometry-parameters\" class=\"anchor\" aria-label=\"Permalink: Geometry parameters\" href=\"#geometry-parameters\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.silentMode\u003c/code\u003e\n[-]\n(Default: False) If true, MCmatlab will not make any command window text outputs during the geometry initialization.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.nx\u003c/code\u003e, \u003ccode\u003emodel.G.ny\u003c/code\u003e, \u003ccode\u003emodel.G.nz\u003c/code\u003e\n[-]\nThe number of bins in the x, y, and z direction, respectively. Higher numbers mean a more finely resolved result, but will also require much longer runtimes to reach a low noise level.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.Lx\u003c/code\u003e, \u003ccode\u003emodel.G.Ly\u003c/code\u003e, \u003ccode\u003emodel.G.Lz\u003c/code\u003e\n[cm]\nThe side lengths of the simulation cuboid, measured in cm.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.mediaPropertiesFunc\u003c/code\u003e\n[-]\nA MATLAB function handle. This should be set to refer to the function at the end of the model file in which the media properties are defined. In principle you could have several different media property functions in your model file and the one referred to in this property is the one that MCmatlab uses, but in practice most model files will be built using only one media property function.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.mediaPropParams\u003c/code\u003e\n[user-defined units]\nA user-defined cell array that you can use to contain all sorts of inputs you would like to use inside the mediaPropertiesFunc. This cell array is useful when doing parametric sweeps (many MC simulations in a for or while loop) in which the media properties vary.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.geomFunc\u003c/code\u003e\n[-]\n(Similar to mediaPropertiesFunc above)\nA MATLAB function handle. This should be set to refer to the function at the end of the model file in which the model geometry is defined. In principle you could have several different geometry functions in your model file and the one referred to in this property is the one that MCmatlab uses, but in practice most model files will be built using only one geometry function.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.geomFuncParams\u003c/code\u003e\n[user-defined units]\n(Similar to mediaPropParams above)\nA user-defined cell array that you can use to contain all sorts of inputs you would like to use inside the geomFunc. This cell array is useful when doing parametric sweeps (many MC simulations in a for or while loop) in which the geometry varies.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e(Excitation) Monte Carlo parameters\u003c/h4\u003e\u003ca id=\"user-content-excitation-monte-carlo-parameters\" class=\"anchor\" aria-label=\"Permalink: (Excitation) Monte Carlo parameters\" href=\"#excitation-monte-carlo-parameters\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.useGPU\u003c/code\u003e\n[-]\n(Default: False)\nIf true, will run the MC simulation on GPU. If false, will use CPU.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.GPUdevice\u003c/code\u003e\n[-]\n(Default: 0)\nThe GPU device to use for GPU accelerated computations. 0 corresponds to the first device. For systems with multiple GPUs, you can launch simulations to different GPUs by varying this property and with the use of, e.g., a MATLAB parallel-for (parfor) loop.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.simulationTimeRequested\u003c/code\u003e\n[minutes]\n(Mutually exclusive with model.MC.nPhotonsRequested)\nThe time to run the MC simualtion for, in minutes. The number of photos launched will vary from run to run.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.nPhotonsRequested\u003c/code\u003e\n[-]\n(Mutually exclusive with model.MC.simulationTimeRequested)\nThe number of photons to launch. The execution time will vary from run to run.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e`model.MC.requestCollectedPhotons\n[-]\n(Default: False)\n(Only used if model.MC.nPhotonsRequested is specified)\nIf true, model.MC.nPhotonsRequested is interpreted as the requested number of collected photon packets, rather than launched photon packets.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.silentMode\u003c/code\u003e\n[-]\n(Default: False)\nIf true, MCmatlab will not make any command window text outputs during the MC simulation.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.useAllCPUs\u003c/code\u003e\n[-]\n(Default: False)\n(Has no effect on MacOS or if model.MC.useGPU = true)\nIf true, MCmatlab will launch a number of threads equal to the number of CPU logical processors on the system. This will lead to the fastest execution but may make the system slow to respond to user inputs (mouse clicks etc.) for the duration of the simulation.\nIf false, MCmatlab will still be multithreaded but will leave one CPU logical processor unused. This will yield almost the same speed of execution but will make the system more responsive while the simulation is running.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.calcNFR\u003c/code\u003e\n[-]\n(Default: True)\nIf true, will calculate and store the normalized fluence rate (NFR) 3D or 4D array (4D if simulating broadband light). The array takes 8*nx*ny*nz*nl bytes of memory (and disk space, if the resulting model file is saved to disk subsequently)\nFor some simulations in which you are only interested, for example, in the detector image/power, you might not need the NFR and could therefore set this to false.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.nExamplePaths\u003c/code\u003e\n[-]\n(Default: 0)\nIf set to a positive integer N, will store the paths of the first N photons for subsequent visualization during the plotting. This is useful to visualize how the photons move around the cuboid.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.farFieldRes\u003c/code\u003e\n[pixels]\n(Default: 0)\nIf set to a positive integer N, MCmatlab will calculate the far field direction angles of the escaping photons and store them in a 2D NxN array (theta,phi on the unit sphere) for later visualization.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.matchedInterfaces\u003c/code\u003e\n[-]\n(Default: True)\nIf true, will set all refractive indices to 1, disregarding any refractive indices specified in the media properties function. In this case, no Fresnel reflection and refraction will be simulated.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.smoothingLengthScale\u003c/code\u003e\n[cm]\n(Only used if matchedInterfaces = false)\nThe characteristic length scale to use for smoothing of the Sobel filter applied to the normal vectors of the non-matched interfaces within the geometry. See\n\u003ca href=\"https://www.spiedigitallibrary.org/journals/journal-of-biomedical-optics/volume-25/issue-02/025001/Modeling-voxel-based-Monte-Carlo-light-transport-with-curved-and/10.1117/1.JBO.25.2.025001.full\" rel=\"nofollow\"\u003ehttps://www.spiedigitallibrary.org/journals/journal-of-biomedical-optics/volume-25/issue-02/025001/Modeling-voxel-based-Monte-Carlo-light-transport-with-curved-and/10.1117/1.JBO.25.2.025001.full\u003c/a\u003e\nfor a description of the technique used.\nThe use of such smoothing enables simulation of reflection and refraction even on oblique interfaces, despite the geometry being defined on a rectangular cuboid mesh. See Example17_CurvedRefractionReflection.m.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.boundaryType\u003c/code\u003e\n[-]\n0: No escaping boundaries\n1: All cuboid boundaries are escaping\n2: Top cuboid boundary only is escaping\n3: Top and bottom boundaries are escaping, while the side boundaries are cyclic\nPhotons that hit a boundary that is \"escaping\" and where the refractive index is equal to 1 will be considered an \"escaped\" photon, and may, depending on the position and direction, be registered by the detector/light collector.\nWhen a photon encounters a boundary that is not escaping, it is allowed to propagate beyond the edge up to a distance of 2½ times the value of (Lx or Ly or Lz) before the photon is finally killed and no longer simulated.\nAllowing photons to propagate beyond the cuboid boundaries enable the photons to potentially scatter back into the simulation volume.\nThe more boundaries are escaping, the faster the simulation will run because fewer photons outside the cuboid have to be simulated.\nWhen a photon hits a cyclic boundary, it will exit and immediately enter the cuboid again on the opposite boundary, as if the cuboid is periodic. In other words, if your geometry and light source is periodically repeating in x and y (such as a simple layered model illuminated by an infinite plane wave), you need only simulate just one unit cell of this pattern and use cyclic x and y boundaries.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.wavelength\u003c/code\u003e\n[nm]\nThe wavelength(s) of the light. May be scalar or 1D array. Media properties in the mediaPropertiesFunc may be dependent on the wavelength of the light. The wavelength does not actually change anything in the MC simulation itself aside from the change in the media properties. Wavelength is also used to calculate the fluorescence emission powers based on the quantum yields of the fluorescers. If wavelength is specified as a 1D array, broadband simulations will be performed.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.sourceType\u003c/code\u003e\n[-]\n(Note that lightSource can be abbreviated LS in your code)\n0: Pencil beam\nA pencil beam is a beam with zero width and zero divergence.\n1: Isotropically emitting line or point source\nThis option is the only one in which the light will originate from within the cuboid. All other options have photons packets starting at the top surface, z = 0.\n2: Infinite plane wave\nA beam with infinite width, but zero divergence.\n3: Laguerre-Gaussian LG01 beam\nA ray-based emulation of the donut-shaped Laguerre-Gaussian LG01 beam.\n4: Radial-factorizable beam\nA beam in which the focus beam profile can be written as I(x,y) = Ir(r), where r = sqrt(x^2+y^2), and similarly for the angular distribution. Circular Gaussian beams can be written in this form.\n5: X/Y factorizable beam\nA beam in which the focus beam profile can be written as I(x,y) = Ix(x)*Iy(y), and similarly for the angular distribution. Rectangular LED emitters can be written in this way, as well as Gaussian (circular and elliptical) beams.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.emitterLength\u003c/code\u003e\n[cm]\n(Only used for model.MC.lightSource.sourceType = 1. Default: 0)\nThe length of the line emitter. If zero, the emitter is a point source.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.focalPlaneIntensityDistribution.radialDistr\u003c/code\u003e\n[-]\n(Note that focalPlaneIntensityDistribution can be abbreviated FPID in your code)\n(Only used for sourceType = 4)\nRadial intensity distribution in the focal plane.\n0: Top-hat\n1: Gaussian\nArray: Custom. Doesn't need to be normalized.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.focalPlaneIntensityDistribution.radialWidth\u003c/code\u003e\n[cm]\n(Note that focalPlaneIntensityDistribution can be abbreviated FPID in your code)\n(Only used for sourceType = 4)\nRadial width of the intensity distribution in the focal plane.\nIf FPID.radialDistr is set to 0 or 1, this is the 1/e^2 radius\nIf FPID.radialDistr is set to an array, this is the half-width of the full distribution\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.focalPlaneIntensityDistribution.XDistr\u003c/code\u003e, \u003ccode\u003emodel.MC.lightSource.focalPlaneIntensityDistribution.YDistr\u003c/code\u003e\n[-]\n(Note that focalPlaneIntensityDistribution can be abbreviated FPID in your code)\n(Only used for sourceType = 5)\nX and Y distribution of the intensity in the focal plane.\n0: Top-hat\n1: Gaussian\nArray: Custom. Doesn't need to be normalized.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.focalPlaneIntensityDistribution.XWidth\u003c/code\u003e, \u003ccode\u003emodel.MC.lightSource.focalPlaneIntensityDistribution.YWidth\u003c/code\u003e\n[cm]\n(Note that focalPlaneIntensityDistribution can be abbreviated FPID in your code)\n(Only used for sourceType = 5)\nX and Y width of the intensity distribution in the focal plane.\nIf FPID.XDistr/FPID.YDistr is set to 0 or 1, this is the 1/e^2 radius\nIf FPID.XDistr/FPID.YDistr is set to an array, this is the half-width of the full distribution\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.angularIntensityDistribution.radialDistr\u003c/code\u003e\n[-]\n(Note that angularIntensityDistribution can be abbreviated AID in your code)\n(Only used for sourceType = 4)\nRadial distribution of the angular intensity.\n0: Top-hat\n1: Gaussian\n2: Cosine (Lambertian)\nArray: Custom. Doesn't need to be normalized.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.angularIntensityDistribution.radialWidth\u003c/code\u003e\n[rad]\n(Note that angularIntensityDistribution can be abbreviated AID in your code)\n(Only used for sourceType = 4 and if AID.radialDistr is not 2)\nRadial width of the angular intensity distribution.\nIf AID.radialDistr is set to 0 or 1, this is the 1/e^2 half-angle.\nIf AID.radialDistr is set to an array, this is the half-angle of the full distribution.\nFor a diffraction limited Gaussian beam, this should be set to model.MC.wavelength*1e-9/(pi*model.MC.lightSource.focalPlaneIntensityDistribution.radialWidth*1e-2))\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.angularIntensityDistribution.XDistr\u003c/code\u003e, \u003ccode\u003emodel.MC.lightSource.angularIntensityDistribution.YDistr\u003c/code\u003e\n[-]\n(Note that angularIntensityDistribution can be abbreviated AID in your code)\n(Only used for sourceType = 5)\nX and Y distribution of the angular intensity.\n0: Top-hat\n1: Gaussian\n2: Cosine (Lambertian)\nArray: Custom. Doesn't need to be normalized.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.angularIntensityDistribution.XWidth\u003c/code\u003e, \u003ccode\u003emodel.MC.lightSource.angularIntensityDistribution.YWidth\u003c/code\u003e\n[rad]\n(Note that angularIntensityDistribution can be abbreviated AID in your code)\n(Only used for sourceType = 5 and if AID.XDistr or AID.YDistr is not 2)\nRadial width of the angular intensity distribution.\nIf AID.XDistr/AID.YDistr is set to 0 or 1, this is the 1/e^2 half-angle.\nIf AID.XDistr/AID.YDistr is set to an array, this is the half-angle of the full distribution.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.xFocus\u003c/code\u003e, \u003ccode\u003emodel.MC.lightSource.yFocus\u003c/code\u003e, \u003ccode\u003emodel.MC.lightSource.zFocus\u003c/code\u003e\n[cm]\nThe focus (or source) position x,y,z coordinates.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.psi\u003c/code\u003e\n[rad]\n(Only used for sourceType = 5. Default: 0)\nAxial rotation angle of the beam.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightSource.theta\u003c/code\u003e, \u003ccode\u003emodel.MC.lightSource.phi\u003c/code\u003e\n[rad]\nPolar and azimuthal angle of the beam center axis.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.sourceDistribution\u003c/code\u003e\n[-]\nIf set to an array of dimensions [nx, ny, nz, nLambda], this will be interpreted as the spatial and spectral distribution of emitters. If this is specified, the contents of lightSource will be disregarded. This array will be normalized by MCmatlab during the call to runMonteCarlo().\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.depositionCriteria.minScatterings\u003c/code\u003e, \u003ccode\u003emodel.MC.depositionCriteria.maxScatterings\u003c/code\u003e, \u003ccode\u003emodel.MC.depositionCriteria.minRefractions\u003c/code\u003e, \u003ccode\u003emodel.MC.depositionCriteria.maxRefractions\u003c/code\u003e, \u003ccode\u003emodel.MC.depositionCriteria.minReflections\u003c/code\u003e, \u003ccode\u003emodel.MC.depositionCriteria.maxReflections\u003c/code\u003e, \u003ccode\u003emodel.MC.depositionCriteria.minInterfaceTransitions\u003c/code\u003e, \u003ccode\u003emodel.MC.depositionCriteria.maxInterfaceTransitions\u003c/code\u003e\n[-]\nThe minimum and maximum number of scattering, refraction, reflection and interface transition events the photon packet must have undergone in order to be registered as an example photon path and to deposit weight into the output arrays (normalized fluence rate, normalized boundary irradiances, image and far field). There is an implied AND between all the criteria. Note that the underlying absorption and propagation of all photon packets are independent of the specified deposition criteria.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.depositionCriteria.minMediumIdxToConsider\u003c/code\u003e, \u003ccode\u003emodel.MC.depositionCriteria.maxMediumIdxToConsider\u003c/code\u003e\n[-]\nThe minimum and maximum medium index that the above deposition criteria apply to. For example, if you've specified minScatterings = 2, minMediumIdxToConsider = 4 and maxMediumIdxToConsider = 5, then only photons that have experienced at least 2 scattering events in media 4 and/or 5 will deposit their weight in the output arrays and register as photon paths. It doesn't matter how many scattering events have happened in other media.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003eInterface transitions and refractions will be considered if the medium transitioned \u003cem\u003einto\u003c/em\u003e has index between minMediumIdxToConsider and maxMediumIdxToConsider.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003eKeep in mind that you can rearrange the media in the media definition and geometry function as required so that the indices of the set of media that you want to consider in deposition criteria are in a contiguous interval.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.depositionCriteria.evaluateOnlyAtEndOfLife\u003c/code\u003e\n[-]\nIf evaluateOnlyAtEndOfLife is false, the photons will only deposit weight into the output arrays and register as photon paths in those segments of the paths where the criteria are satisfied. If it is true, weight is deposited and path is registered along the full path if the criteria are satisfied at the end of the photon's life span.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.depositionCriteria.onlyCollected\u003c/code\u003e\n[-]\nIf evaluateOnlyAtEndOfLife is true, you may also specify onlyCollected. It is an extra criterion that states that the photon must have been collected on the light collector.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.P\u003c/code\u003e\n[W]\n(Default: 1)\n(Only used for the thermal simulations and for any Monte Carlo simulations in which the optical or thermal parameters depend on the fluence rate (FR), fractional damage (FD) or temperature (T))\nIncident pulse peak power. In case of infinite plane waves, this is only the power incident upon the cuboid's top surface.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.spectrumFunc\u003c/code\u003e\n[-]\n(Default: 1)\n(Only used for broadband simulations)\nA function handle that takes wavelength as an input and returns the spectral power of the source as an output. This function doesn't need to be normalized, as the total power emitted across all simulated wavelengths will be normalized to \u003ccode\u003emodel.MC.P\u003c/code\u003e regardless.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.FRinitial\u003c/code\u003e\n[W/cm^2]\n(Only used for MC simulations in which the optical properties depend on the fluence rate (FR))\nInitial guess for the fluence rate distribution in, to be used for iterative fluence rate dependent simulations.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.FRdepIterations\u003c/code\u003e\n[-]\n(Only used for MC simulations in which the optical properties depend on the fluence rate (FR))\nThe number of iterations (times the MC simulation needs to be run) each time a new calculation of the MC outputs is requested.\nTest for yourself how high this number needs to be for your model. In my tests, 20 was enough.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.useLightCollector\u003c/code\u003e\n[-]\n(Default: False)\nA logical (boolean) to specify whether the MC simulation should keep track of whether photons hit the light collector/detector.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e(The following LC properties are only used if useLightCollector = true)\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.f\u003c/code\u003e\n[cm]\n(Note that lightCollector can be abbreviated LC in your code)\nIf the light collector is supposed to be an objective lens, this is its focal length.\nIf the light collector is supposed to be a fiber tip this should be set to Inf (infinity)\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.x\u003c/code\u003e, \u003ccode\u003emodel.MC.lightCollector.y\u003c/code\u003e, \u003ccode\u003emodel.MC.lightCollector.z\u003c/code\u003e\n[cm]\n(Note that lightCollector can be abbreviated LC in your code)\nIf model.MC.lightCollector.f is finite (light collector is an objective lens), this is the x, y, z position of the center of the focal plane of the objective lens.\nIf model.MC.lightCollector.f is infinite (light collector is a fiber tip), this is the x, y, z position of the center of the fiber tip.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.theta\u003c/code\u003e, \u003ccode\u003emodel.MC.lightCollector.phi\u003c/code\u003e\n[rad]\n(Note that lightCollector can be abbreviated LC in your code)\nPolar and azimuthal angle of direction that the light collector is facing\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.NA\u003c/code\u003e\n[-]\n(Note that lightCollector can be abbreviated LC in your code)\n(Only used for infinite f)\nFiber numerical aperture.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.diam\u003c/code\u003e\n[cm]\n(Note that lightCollector can be abbreviated LC in your code)\nDiameter of the light collector aperture. For an ideal thin lens with numerical aperture NA, this is 2f*tan(asin(NA)).\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.fieldSize\u003c/code\u003e\n[cm]\n(Note that lightCollector can be abbreviated LC in your code)\n(Only used for finite f)\nField size of the imaging system, that is, the diameter of area in object plane that gets imaged.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.res\u003c/code\u003e\n[pixels]\n(Note that lightCollector can be abbreviated LC in your code)\n(Only used for finite f)\nX and Y resolution of light collector, only used for finite f\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.tStart\u003c/code\u003e, \u003ccode\u003emodel.MC.lightCollector.tEnd\u003c/code\u003e\n[s]\n(Note that lightCollector can be abbreviated LC in your code)\nStart and end time of the detection time-of-flight interval. Note that photons arriving before tStart will still be registered but all binned together in a single bin containing all \"too-early\" photons. Likewise, all photons arriving after tEnd are binned into a \"too-late\" bin.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.nTimeBins\u003c/code\u003e\n[-]\n(Note that lightCollector can be abbreviated LC in your code)\n(Default: 0)\nNumber of bins between tStart and tEnd. If zero, the measurement is not time-resolved.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eFluorescence Monte Carlo parameters\u003c/h4\u003e\u003ca id=\"user-content-fluorescence-monte-carlo-parameters\" class=\"anchor\" aria-label=\"Permalink: Fluorescence Monte Carlo parameters\" href=\"#fluorescence-monte-carlo-parameters\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eThe following properties exist for fluorescence Monte Carlo simulations, and they work the same as for regular MC simulations:\n\u003ccode\u003eFMC.useGPU\u003c/code\u003e, \u003ccode\u003eFMC.GPUdevice\u003c/code\u003e, \u003ccode\u003eFMC.simulationTimeRequested\u003c/code\u003e, \u003ccode\u003eFMC.nPhotonsRequested\u003c/code\u003e, \u003ccode\u003eFMC.silentMode\u003c/code\u003e, \u003ccode\u003eFMC.useAllCPUs\u003c/code\u003e, \u003ccode\u003eFMC.calcNormalizedFluenceRate\u003c/code\u003e, \u003ccode\u003eFMC.nExamplePaths\u003c/code\u003e, \u003ccode\u003eFMC.farFieldRes\u003c/code\u003e, \u003ccode\u003eFMC.matchedInterfaces\u003c/code\u003e, \u003ccode\u003eFMC.smoothingLengthScale\u003c/code\u003e, \u003ccode\u003eFMC.boundaryType\u003c/code\u003e, \u003ccode\u003eFMC.wavelength\u003c/code\u003e, \u003ccode\u003eFMC.useLightCollector\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.x\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.y\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.z\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.theta\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.phi\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.f\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.diam\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.fieldSize\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.NA\u003c/code\u003e, \u003ccode\u003eFMC.lightCollector.res\u003c/code\u003e\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eHeat solver parameters\u003c/h4\u003e\u003ca id=\"user-content-heat-solver-parameters\" class=\"anchor\" aria-label=\"Permalink: Heat solver parameters\" href=\"#heat-solver-parameters\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.useGPU\u003c/code\u003e\n[-]\n(Default: false)\nUse CUDA acceleration for the heat simulation solver for NVIDIA GPUs\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.silentMode\u003c/code\u003e\n[-]\n(Default: false)\nIf true, MCmatlab will not make any command window text outputs during the heat simulation.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.useAllCPUs\u003c/code\u003e\n[-]\n(Default: false)\n(Has no effect on MacOS or if model.MC.useGPU = true)\nIf true, MCmatlab will launch a number of threads equal to the number of CPU logical processors on the system. This will lead to the fastest execution but may make the system slow to respond to user inputs (mouse clicks etc.) for the duration of the simulation.\nIf false, MCmatlab will launch will still be multithreaded but will leave one CPU logical processor unused. This will yield almost the same speed of execution but will make the system more responsive while the simulation is running.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.makeMovie\u003c/code\u003e\n[-]\n(Default: false)\n(Only used if silentMode = false)\nIf true, MCmatlab will record each frame of the volumetric temperature plot and get ready to save the frames to a movie file.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.deferMovieWrite\u003c/code\u003e\n[-]\n(Default: false)\n(Only used if silentMode = false and makeMovie = true)\nIf false, MCmatlab will save the recorded frames to a movie file. If true, the frames are still stored within the model object so that subsequent heat simulations can be concatenated to them before saving.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.largeTimeSteps\u003c/code\u003e\n[-]\n(Default: false)\nIf true, calculations will be faster, but some voxel temperatures may be slightly less precise. Test for yourself whether this precision is acceptable for your application.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.heatBoundaryType\u003c/code\u003e\n[-]\nThe type of boundary condition to use for the heat solver.\n0: Insulating boundaries\n1: Constant-temperature boundaries (heat-sinked)\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.nPulses\u003c/code\u003e\n[-]\nNumber of consecutive pulses, each with an illumination phase and a diffusion phase. If simulating only illumination or only diffusion, use nPulses = 1.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.durationOn\u003c/code\u003e, \u003ccode\u003emodel.HS.durationOff\u003c/code\u003e\n[s]\nPulse on-duration and off-duration\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.durationEnd\u003c/code\u003e\n[s]\nNon-illuminated relaxation time to add to the end of the simulation to let temperature diffuse after the pulse train.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.T\u003c/code\u003e\n[deg C]\n(Functions both as an input and an output property)\nInitial and final temperature, can be scalar or 3D array of dimensions nx, ny, nz.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.plotTempLimits\u003c/code\u003e\n[deg C]\nAn array of two values designating the expected range of temperatures, used only for setting the color scale in the plot. One or both values can be NaN to let the limit be set to the minimum or maximum of the data. For example [NaN 100] means the lower color limit is automatically set to the minimum value in the data, but the upper color limit is fixed at 100.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.nUpdates\u003c/code\u003e\n[-]\nNumber of times data is extracted for plots during each pulse. A minimum of 1 update is performed in each phase (2 for each pulse consisting of an illumination phase and a diffusion phase)\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.mediaPropRecalcPeriod\u003c/code\u003e\n[-]\n(Used only if optical or thermal parameters have been specified to be dependent on temperature (T))\nEvery time this many updates have passed, the media properties will be recalculated (including, if needed, re-running MC and FMC steps). Check that this is low enough to ensure convergence of your results.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.slicePositions\u003c/code\u003e\n[-]\n(Default: [0.5 1 1])\nAn array of three values, describing the fractional x, y, z positions on a scale from 0 to 1 to place the volumetric slices at.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.tempSensorPositions\u003c/code\u003e\n[cm]\n(Default: empty array)\nA 2D array with three columns.\nEach row describes the x, y, z coordinates of a temperature sensor placed within the cuboid, at which the temperature will be recorded for subsequent plotting as a function of time.\nLeave the matrix empty ([]) to disable temperature sensors.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch3 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eList and explanation of output properties\u003c/h3\u003e\u003ca id=\"user-content-list-and-explanation-of-output-properties\" class=\"anchor\" aria-label=\"Permalink: List and explanation of output properties\" href=\"#list-and-explanation-of-output-properties\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eAs in the previous section, we assume that the model object variable has been named \"model\". In principle, it could be given any name you want.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eGeometry properties\u003c/h4\u003e\u003ca id=\"user-content-geometry-properties\" class=\"anchor\" aria-label=\"Permalink: Geometry properties\" href=\"#geometry-properties\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.dx\u003c/code\u003e, \u003ccode\u003emodel.G.dy\u003c/code\u003e, \u003ccode\u003emodel.G.dz\u003c/code\u003e\n[cm]\nThe side lengths of the voxels. They are simply calculated as the side length of the simulation cuboid divided by the number of bins, for example, model.G.Lx/model.G.nx.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.x\u003c/code\u003e, \u003ccode\u003emodel.G.y\u003c/code\u003e, \u003ccode\u003emodel.G.z\u003c/code\u003e\n[cm]\n1D arrays with the x, y or z coordinate values corresponding to the centers of the voxels\nYou can use these for easy plotting of slices, see for example the entry on NFR in the MC section below.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.G.M_raw\u003c/code\u003e\n[-]\n3D (xyz) array in coordinate order of the tissue indices as calculated from the geomFunc. This is the array that is plotted in the figure called Geometry Illustration.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003e(Excitation) Monte Carlo properties\u003c/h4\u003e\u003ca id=\"user-content-excitation-monte-carlo-properties\" class=\"anchor\" aria-label=\"Permalink: (Excitation) Monte Carlo properties\" href=\"#excitation-monte-carlo-properties\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.simulationTime\u003c/code\u003e\n[min]\nThe actual simulation time of the most recent Monte Carlo simulation run. If you did not define model.MC.nPhotonsRequested, then the simulation is timed and model.MC.simulationTime should be very close to `model.MC.simulationTimeRequested.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.nPhotons\u003c/code\u003e\n[-]\nThe actual number of photon packets launched in the most recent Monte Carlo simulation run. If you defined model.MC.nPhotonsRequested, then model.MC.nPhotons will be equal to that number.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.nPhotonsCollected\u003c/code\u003e\n[-]\nThe actual number of photon packets that was registered on the light collected in the most recent Monte Carlo simulation run. If you set model.MC.requestCollectedPhotons = true, then model.MC.nPhotonsCollected will be equal to model.MC.nPhotonsRequested.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.mediaProperties\u003c/code\u003e\n[-]\nA struct that contains the media properties as evaluated at the specified excitation Monte Carlo wavelength, model.MC.wavelength.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.M\u003c/code\u003e\n[-]\nA 3D (xyz) array. If the media properties do not contain dependences on fluence rate (FR), temperature (T) or fractional damage (FD), then this array will simply be equal to model.G.M_raw. Otherwise, model.MC.M will be the \"split\" version of model.G.M_raw, in which those media that have dependences have been split into the specified number of sub-media with different optical/thermal properties for the purposes of the simulations.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.interfaceNormals\u003c/code\u003e\n[-]\nA 2D array of dimension (2 x (nx\u003cem\u003eny\u003c/em\u003enz)) where local interface normal vector angles are stored. Each column contains the theta, phi angles for one voxel's interface normal vector. Used for calculated of refraction and reflection on oblique and curved interfaces between media with different refractive index.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.examplePaths\u003c/code\u003e\n[cm] and [-]\nA 2D array which stores the example paths' coordinates and remaining weight. Each column is a data point where the first three rows are the x, y, z position of the photon packet and the fourth row is the remaining weight (energy) of the photon packet. Different photon trajectories are separated by a column of NaNs.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.normalizedFluenceRate\u003c/code\u003e\n[W/cm^2/W.incident]\n(Note that normalizedFluenceRate can be abbreviated NFR in your code)\nA 3D or 4D array (4D if simulating broadband light) (x,y,z,lambda) of normalized fluence rate values. This is what's plotted in figure 4. If you want to plot a slice out of this distribution, you could for example do it with these three lines of code:\u003c/p\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003e\u003ccode\u003eNFRslice = squeeze(model.MC.NFR(51,:,:));\u003c/code\u003e Extracts the slice corresponding to the 51st x value. \u003ccode\u003esqueeze\u003c/code\u003e is to remove the x singleton dimension, giving you a 2D (yz) array of normalized fluence rates.\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003efigure(100);\u003c/code\u003e\u003c/li\u003e\n\u003cli\u003e\u003ccode\u003eimagesc(model.G.y,model.G.z,NFRslice.');\u003c/code\u003e We can use the 1D coordinate arrays from model.G for the y and z coordinate values. The \u003ccode\u003e.'\u003c/code\u003e is there because Mathworks has designed the imagesc function to plot the first coordinate along the vertical axis and the second coordinate along the horizontal axis, which is the opposite of what we want.\u003c/li\u003e\n\u003c/ul\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.normalizedAbsorption\u003c/code\u003e\n[W/cm^3/W.incident]\n(Note that normalizedAbsorption can be abbreviated NA in your code)\nA 3D or 4D array (4D if simulating broadband light) (x,y,z,lambda) of normalized absorption values. This is what's plotted in figure 3.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.farField\u003c/code\u003e\n[W/sr/W.incident]\nA 2D or 3D (theta,phi,lambda) array of normalized radiant intensity values for the light that escaped the simulation cuboid. The axes are the polar and azimuthal angles, described below.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.farFieldTheta\u003c/code\u003e\n[rad]\nA 1D array of polar angles corresponding to the first dimension of model.MC.farField.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.farFieldPhi\u003c/code\u003e\n[rad]\nA 1D array of azimuthal angles corresponding to the second dimension of model.MC.farField.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.normalizedIrradiance_xpos\u003c/code\u003e, \u003ccode\u003emodel.MC.normalizedIrradiance_xneg\u003c/code\u003e, \u003ccode\u003emodel.MC.normalizedIrradiance_ypos\u003c/code\u003e, \u003ccode\u003emodel.MC.normalizedIrradiance_yneg\u003c/code\u003e, \u003ccode\u003emodel.MC.normalizedIrradiance_zpos\u003c/code\u003e, \u003ccode\u003emodel.MC.normalizedIrradiance_zneg\u003c/code\u003e\n[W/cm^2/W.incident]\n(Note that normalizedIrradiance can be abbreviated NI in your code)\n2D or 3D (xy, xz or yz - with lambda as third dimension) arrays of normalized irradiances of the light hitting the boundaries (either escaping or killed). For example, the property named \u003ccode\u003emodel.MC.NI_xpos\u003c/code\u003e designates the light that hits the surface that is orthogonal to the x axis and placed on the positive x side, whereas the \u003ccode\u003emodel.MC.NI_xneg\u003c/code\u003e refers to the surface orthogonal to the x axis and placed on the negative x side. model.MC.boundaryType determine which of these arrays are calculated.\n\u003ccode\u003emodel.MC.NI_zneg\u003c/code\u003e is of special interest to users interested in calculating the reflectance, which can be found as the integral over the array:\u003c/p\u003e\n\u003cul dir=\"auto\"\u003e\n\u003cli\u003e\u003ccode\u003eR = model.G.dx*model.G.dy*sum(model.MC.NI_zneg(:));\u003c/code\u003e\u003c/li\u003e\n\u003c/ul\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.MC.lightCollector.image\u003c/code\u003e\n[W/cm^2/W.incident]\nIf \u003ccode\u003emodel.MC.lightCollector.res == 1\u003c/code\u003e, this is a scalar or 1D array with the normalized power registered on the light collector as function of wavelength.\nIf \u003ccode\u003emodel.MC.lightCollector.res \u0026gt; 1\u003c/code\u003e, this is a 2D or 3D array (X,Y,lambda) of normalized irradiances registered on the light collector. This array describes the light distribution you would get on a camera looking at the cuboid through an objective lens.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eFluorescence Monte Carlo properties\u003c/h4\u003e\u003ca id=\"user-content-fluorescence-monte-carlo-properties\" class=\"anchor\" aria-label=\"Permalink: Fluorescence Monte Carlo properties\" href=\"#fluorescence-monte-carlo-properties\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eAll the output properties described above for excitation Monte Carlo are also provided for fluorescence Monte Carlo in the model.FMC object.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch4 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eHeat solver properties\u003c/h4\u003e\u003ca id=\"user-content-heat-solver-properties\" class=\"anchor\" aria-label=\"Permalink: Heat solver properties\" href=\"#heat-solver-properties\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.M\u003c/code\u003e\n[-]\nA 3D (xyz) array. If the media properties do not contain dependences on fluence rate (FR), temperature (T) or fractional damage (FD), then this array will simply be equal to model.G.M_raw. Otherwise, model.HS.M will be the \"split\" version of model.G.M_raw, in which those media that have dependences have been split into the specified number of sub-media with different optical/thermal properties for the purposes of the simulations.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.T\u003c/code\u003e\n[deg C]\nA 3D (xyz) array with the final temperature values of the simulation.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.Omega\u003c/code\u003e\n[-]\nA 3D (xyz) array with the final Omega values of the simulation. Omega describes the thermally induced tissue damage calculated according to the Arrhenius damage integral.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.maxMediaTemps\u003c/code\u003e\n[deg C]\nA 1D array that contains the maximal temperatures obtained in each tissue type involved in the simulation.\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.sensorsTimeVector\u003c/code\u003e\n[s]\nA 1D array of time values that should be used for plotting the sensorTemps data (see below).\u003c/p\u003e\n\u003cp dir=\"auto\"\u003e\u003ccode\u003emodel.HS.sensorTemps\u003c/code\u003e\n[deg C]\nA 2D array of temperatures measured at the specified sensor positions. Each row corresponds to one sensor. Use the model.HS.sensorsTimeVector as the time values when plotting this data.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch2 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eContribution guidelines\u003c/h2\u003e\u003ca id=\"user-content-contribution-guidelines\" class=\"anchor\" aria-label=\"Permalink: Contribution guidelines\" href=\"#contribution-guidelines\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eYou are very welcome to clone the repository and add features of your own. If you want to report a bug or are missing a feature, shoot me an email, see below.\u003c/p\u003e\n\u003cdiv class=\"markdown-heading\" dir=\"auto\"\u003e\u003ch2 tabindex=\"-1\" class=\"heading-element\" dir=\"auto\"\u003eWho do I talk to?\u003c/h2\u003e\u003ca id=\"user-content-who-do-i-talk-to\" class=\"anchor\" aria-label=\"Permalink: Who do I talk to?\" href=\"#who-do-i-talk-to\"\u003e\u003csvg class=\"octicon octicon-link\" viewBox=\"0 0 16 16\" version=\"1.1\" width=\"16\" height=\"16\" aria-hidden=\"true\"\u003e\u003cpath d=\"m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z\"\u003e\u003c/path\u003e\u003c/svg\u003e\u003c/a\u003e\u003c/div\u003e\n\u003cp dir=\"auto\"\u003eThe main person responsible for MCmatlab is Anders Kragh Hansen: \u003ca href=\"mailto:anderskraghhansen@gmail.com\"\u003eanderskraghhansen@gmail.com\u003c/a\u003e\u003c/p\u003e\n\u003c/article\u003e","loaded":true,"timedOut":false,"errorMessage":null,"headerInfo":{"toc":[{"level":1,"text":"Readme and User Manual for MCmatlab","anchor":"readme-and-user-manual-for-mcmatlab","htmlText":"Readme and User Manual for MCmatlab"},{"level":2,"text":"What is MCmatlab?","anchor":"what-is-mcmatlab","htmlText":"What is MCmatlab?"},{"level":2,"text":"License","anchor":"license","htmlText":"License"},{"level":2,"text":"How do I get set up?","anchor":"how-do-i-get-set-up","htmlText":"How do I get set up?"},{"level":3,"text":"Requirements","anchor":"requirements","htmlText":"Requirements"},{"level":3,"text":"Helper files","anchor":"helper-files","htmlText":"Helper files"},{"level":2,"text":"How do I use MCmatlab?","anchor":"how-do-i-use-mcmatlab","htmlText":"How do I use MCmatlab?"},{"level":3,"text":"Compilation","anchor":"compilation","htmlText":"Compilation"},{"level":3,"text":"Model files","anchor":"model-files","htmlText":"Model files"},{"level":3,"text":"Model object","anchor":"model-object","htmlText":"Model object"},{"level":3,"text":"MATLAB function definitions","anchor":"matlab-function-definitions","htmlText":"MATLAB function definitions"},{"level":3,"text":"Media properties","anchor":"media-properties","htmlText":"Media properties"},{"level":3,"text":"Building the model","anchor":"building-the-model","htmlText":"Building the model"},{"level":4,"text":"1. Build geometry","anchor":"1-build-geometry","htmlText":"1. Build geometry"},{"level":4,"text":"2. Calculate light distribution","anchor":"2-calculate-light-distribution","htmlText":"2. Calculate light distribution"},{"level":4,"text":"3. (Optional) Include Fresnel reflection and refraction","anchor":"3-optional-include-fresnel-reflection-and-refraction","htmlText":"3. (Optional) Include Fresnel reflection and refraction"},{"level":4,"text":"4. (Optional) Calculate fluorescence light distribution","anchor":"4-optional-calculate-fluorescence-light-distribution","htmlText":"4. (Optional) Calculate fluorescence light distribution"},{"level":4,"text":"5. (Optional) Simulate heat distribution","anchor":"5-optional-simulate-heat-distribution","htmlText":"5. (Optional) Simulate heat distribution"},{"level":4,"text":"6. (Optional) Imaging: Model the intensity distribution received by a detector/light collector","anchor":"6-optional-imaging-model-the-intensity-distribution-received-by-a-detectorlight-collector","htmlText":"6. (Optional) Imaging: Model the intensity distribution received by a detector/light collector"},{"level":4,"text":"7. (Optional) Calculate the far field angular distribution of light escaping the simulation volume","anchor":"7-optional-calculate-the-far-field-angular-distribution-of-light-escaping-the-simulation-volume","htmlText":"7. (Optional) Calculate the far field angular distribution of light escaping the simulation volume"},{"level":4,"text":"8. (Optional) Use deposition criteria to show the normalized fluence rate array of only those photons which end up on the detector","anchor":"8-optional-use-deposition-criteria-to-show-the-normalized-fluence-rate-array-of-only-those-photons-which-end-up-on-the-detector","htmlText":"8. (Optional) Use deposition criteria to show the normalized fluence rate array of only those photons which end up on the detector"},{"level":4,"text":"9. (Optional) Programmatically assign values to the parameters","anchor":"9-optional-programmatically-assign-values-to-the-parameters","htmlText":"9. (Optional) Programmatically assign values to the parameters"},{"level":4,"text":"10. (Optional) Define fluence rate-, temperature- or fractional damage-dependent optical or thermal properties","anchor":"10-optional-define-fluence-rate--temperature--or-fractional-damage-dependent-optical-or-thermal-properties","htmlText":"10. (Optional) Define fluence rate-, temperature- or fractional damage-dependent optical or thermal properties"},{"level":4,"text":"11. (Optional) Enable CUDA GPU acceleration","anchor":"11-optional-enable-cuda-gpu-acceleration","htmlText":"11. (Optional) Enable CUDA GPU acceleration"},{"level":3,"text":"List and explanation of input parameters","anchor":"list-and-explanation-of-input-parameters","htmlText":"List and explanation of input parameters"},{"level":4,"text":"Geometry parameters","anchor":"geometry-parameters","htmlText":"Geometry parameters"},{"level":4,"text":"(Excitation) Monte Carlo parameters","anchor":"excitation-monte-carlo-parameters","htmlText":"(Excitation) Monte Carlo parameters"},{"level":4,"text":"Fluorescence Monte Carlo parameters","anchor":"fluorescence-monte-carlo-parameters","htmlText":"Fluorescence Monte Carlo parameters"},{"level":4,"text":"Heat solver parameters","anchor":"heat-solver-parameters","htmlText":"Heat solver parameters"},{"level":3,"text":"List and explanation of output properties","anchor":"list-and-explanation-of-output-properties","htmlText":"List and explanation of output properties"},{"level":4,"text":"Geometry properties","anchor":"geometry-properties","htmlText":"Geometry properties"},{"level":4,"text":"(Excitation) Monte Carlo properties","anchor":"excitation-monte-carlo-properties","htmlText":"(Excitation) Monte Carlo properties"},{"level":4,"text":"Fluorescence Monte Carlo properties","anchor":"fluorescence-monte-carlo-properties","htmlText":"Fluorescence Monte Carlo properties"},{"level":4,"text":"Heat solver properties","anchor":"heat-solver-properties","htmlText":"Heat solver properties"},{"level":2,"text":"Contribution guidelines","anchor":"contribution-guidelines","htmlText":"Contribution guidelines"},{"level":2,"text":"Who do I talk to?","anchor":"who-do-i-talk-to","htmlText":"Who do I talk 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0 1 1 0 0 1 2 0ZM2 4a1 1 0 1 1 0-2 1 1 0 0 1 0 2Z"></path></svg></button></div><div class="Box-sc-g0xbh4-0 QkQOb js-snippet-clipboard-copy-unpositioned undefined" data-hpc="true"><article class="markdown-body entry-content container-lg" itemprop="text"><div class="markdown-heading" dir="auto"><h1 tabindex="-1" class="heading-element" dir="auto">Readme and User Manual for MCmatlab</h1><a id="user-content-readme-and-user-manual-for-mcmatlab" class="anchor" aria-label="Permalink: Readme and User Manual for MCmatlab" href="#readme-and-user-manual-for-mcmatlab"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <div class="markdown-heading" dir="auto"><h2 tabindex="-1" class="heading-element" dir="auto">What is MCmatlab?</h2><a id="user-content-what-is-mcmatlab" class="anchor" aria-label="Permalink: What is MCmatlab?" href="#what-is-mcmatlab"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">MCmatlab is a Monte Carlo simulation for modeling light propagation in a 3D voxel space. Fluorescence can optionally be simulated after simulation of the excitation light. Included is also a finite element simulation for temperature increase and heat diffusion in the same voxel space.</p> <p dir="auto">Primarily targeted for tissue optics, but can be used in any environment with turbid media in which the wave nature of light (interference phenomena) is negligible and a ray-tracing model is appropriate.</p> <p dir="auto">You can find the latest version of MCmatlab on <a href="https://github.com/ankrh/MCmatlab">https://github.com/ankrh/MCmatlab</a>. You can also use MCmatlab directly in MATLAB online by clicking the button below. If you publish results obtained with this software, we would be thankful if you cited its accompanying article: doi:10.1117/1.JBO.23.12.121622</p> <p dir="auto"><a href="https://matlab.mathworks.com/open/github/v1?repo=ankrh/MCmatlab&amp;file=Example1_StandardTissue.m" rel="nofollow"><img src="https://camo.githubusercontent.com/2f3855e7dfae2344a326fab483b2599adfb2151c0630878b1deda2433bc5a8d4/68747470733a2f2f7777772e6d617468776f726b732e636f6d2f696d616765732f726573706f6e736976652f676c6f62616c2f6f70656e2d696e2d6d61746c61622d6f6e6c696e652e737667" alt="Open in MATLAB Online" data-canonical-src="https://www.mathworks.com/images/responsive/global/open-in-matlab-online.svg" style="max-width: 100%;"></a></p> <div class="markdown-heading" dir="auto"><h2 tabindex="-1" class="heading-element" dir="auto">License</h2><a id="user-content-license" class="anchor" aria-label="Permalink: License" href="#license"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see <a href="https://www.gnu.org/licenses/" rel="nofollow">https://www.gnu.org/licenses/</a>.</p> <div class="markdown-heading" dir="auto"><h2 tabindex="-1" class="heading-element" dir="auto">How do I get set up?</h2><a id="user-content-how-do-i-get-set-up" class="anchor" aria-label="Permalink: How do I get set up?" href="#how-do-i-get-set-up"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">Requirements</h3><a id="user-content-requirements" class="anchor" aria-label="Permalink: Requirements" href="#requirements"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>Windows 7, macOS 10.12 (Sierra) or newer or Linux</li> <li>MATLAB R2018a or newer (only the intel-versions of MATLAB are supported)</li> <li>(For GPU accelerated computation) A Windows PC with a CUDA-enabled graphics card and the MATLAB Parallel Computing Toolbox</li> </ul> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">Helper files</h3><a id="user-content-helper-files" class="anchor" aria-label="Permalink: Helper files" href="#helper-files"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">All the helper functions needed for running MCmatlab are located in the folder (MATLAB package) "+MCmatlab", and its parent folder therefore has to be on your MATLAB path when trying to run any MCmatlab model files. You will not need to modify any of the contained files. We recommend keeping the model files in a folder together with the "+MCmatlab" folder, such that you don't need to manually add the parent folder of "+MCmatlab" to your MATLAB path.</p> <div class="markdown-heading" dir="auto"><h2 tabindex="-1" class="heading-element" dir="auto">How do I use MCmatlab?</h2><a id="user-content-how-do-i-use-mcmatlab" class="anchor" aria-label="Permalink: How do I use MCmatlab?" href="#how-do-i-use-mcmatlab"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">Compilation</h3><a id="user-content-compilation" class="anchor" aria-label="Permalink: Compilation" href="#compilation"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">The folders include all the executables necessary, so you don't need to compile anything. If, however, you want to change the routine in either the MCmatlab.c source code or the finiteElementHeatPropagator.c source code (both located in the folder "+MCmatlab/src"), you will need to recompile the respective mex-files. Check out those two source-files on how to do so. The source code is written in such a way that it can be compiled as either C or C++ code using either GCC, MSVC, clang or as CUDA source code using NVCC.</p> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">Model files</h3><a id="user-content-model-files" class="anchor" aria-label="Permalink: Model files" href="#model-files"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">In MCmatlab, you set up your model in a single m-file called "Model File". You can find some examples of Model Files to get you started in the parent folder of "+MCmatlab". A complete list of parameters that can be set is provided below.</p> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">Model object</h3><a id="user-content-model-object" class="anchor" aria-label="Permalink: Model object" href="#model-object"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">A "Model Object" stores all the parameters for a single Monte Carlo simulation: a single geometry and a single type of lightsource, together with all the results from the Monte Carlo (and optional heat transfer) simulation. The Model Object is an instance of the class MCmatlab.model, i.e., it's of the class "model" in the MATLAB-package "MCmatlab". One Model File can, if desired, generate multiple Model Objects with a different geometry and/or lightsource each.</p> <p dir="auto">Model Objects can be saved to and loaded from a standard binary MATLAB MAT-file like any other MATLAB variable. When loading a Model Object from a MATLAB MAT-file, the parent folder of "+MCmatlab" needs to be on your MATLAB path: prior to loading the Model Object, either navigate to the parent folder of "+MCmatlab" in the "Current Folder" view of MATLAB, or use the command "addpath" to add the parent folder of "+MCmatlab" to your path.</p> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">MATLAB function definitions</h3><a id="user-content-matlab-function-definitions" class="anchor" aria-label="Permalink: MATLAB function definitions" href="#matlab-function-definitions"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">MCmatlab makes extensive use of user-defined functions, passed into the simulation in the form of function handles. For more information, see <code>https://www.mathworks.com/help/matlab/matlab_prog/creating-a-function-handle.html</code>. Inside other functions, nested functions can be defined anywhere, but in the main model file script, MATLAB requires that all functions are defined at the end of the m file.</p> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">Media properties</h3><a id="user-content-media-properties" class="anchor" aria-label="Permalink: Media properties" href="#media-properties"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">The optical properties of all media are defined in a function at the end of the model file. The examples contain some media you can modify or copy-paste to your own model file, or you define your own media from scratch in your own models. All media properties functions must start with this line: <code>mediaProperties = MCmatlab.mediumProperties;</code> in order to initialize the <code>mediaProperties</code> variable as an array of <code>mediumProperties</code> objects. Make sure that each media in a single model file has its distinct "j"-number, as this is the number you will refer to when building your model in the geometry function (see below).</p> <p dir="auto">Each medium can be specified with up to 13 properties. Many of these may be specified either as a scalar or as function handles that can take wavelength, fluence rate (FR), temperature (T) and fractional damage (FD) as input:</p> <ul dir="auto"> <li><code>name</code> - A char array containing the name of the medium, used for the visualization.</li> <li><code>mua</code> - The absorption coefficient in units of 1/cm. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.</li> <li><code>mus</code> - The scattering coefficient in units of 1/cm. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.</li> <li><code>g</code> - The scattering anisotropy (the mean cosine to the scattering angle), to be used in the Henyey-Greenstein phase function. It has no units. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.</li> <li><code>customPhaseFunc</code> - An alternative to specifying <code>g</code>. If specified, this must be a function handle that takes wavelength and polar scattering angle as inputs and yields the scattering phase function as output. This function does not need to be normalized.</li> <li><code>n</code> - The refractive index. May be (a) scalar or (b) a function handle taking wavelength as input.</li> <li><code>QY</code> - The quantum yield of fluorescence, that is, photons of fluorescence emitted relative to excitation photons absorbed. It has no units. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.</li> <li><code>ES</code> - The emission spectrum of the fluorescence emission, if any. Doesn't need to be normalized. May be (a) scalar, (b) a function handle taking wavelength as input or (c) a function handle taking wavelength, FR, T and FD as inputs.</li> <li><code>VHC</code> - The volumetric heat capacity of the medium in units of J/(cm^3 K). May be (a) scalar or (b) a function handle taking T and FD as inputs.</li> <li><code>TC</code> - The thermal conductivity of the medium in units of W/(cm K). May be (a) scalar or (b) a function handle taking T and FD as inputs.</li> <li><code>E</code> - The Arrhenius activation energy in units of J/mol. Must be scalar.</li> <li><code>A</code> - The Arrhenius pre-exponential factor in units of 1/s. Must be scalar.</li> <li><code>nBins</code> - The number of bins (sub-media) to split the medium into in case of media that have properties that depend on fluence rate (FR), temperature (T) or fractional damage (FD). Must be scalar.</li> </ul> <p dir="auto">For Monte Carlo simulations, <code>name</code>, <code>mua</code>, <code>mus</code> and either <code>g</code> or <code>customPhaseFunc</code> need be specified for all media.</p> <p dir="auto">For fluorescence Monte Carlo simulations, the <code>QY</code> and <code>ES</code> properties must additionally be specified for those media that fluoresce.</p> <p dir="auto">For heat simulations, <code>VHC</code> and <code>TC</code> must be specified for all media.</p> <p dir="auto">For heat simulations with calculation of tissue damage, <code>E</code> and <code>A</code> must be specified for those media that can be damaged.</p> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">Building the model</h3><a id="user-content-building-the-model" class="anchor" aria-label="Permalink: Building the model" href="#building-the-model"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">You build each model in a separate m-file. Each model requires the first two and optionally more of the following steps:</p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">1. Build geometry</h4><a id="user-content-1-build-geometry" class="anchor" aria-label="Permalink: 1. Build geometry" href="#1-build-geometry"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>Modify or add to "mediaPropertiesFunc" at the end of the model file to include the definitions of the media you're interested in. You may optionally include thermal and/or fluorescence properties.</li> <li>In your model file, specify the side lengths Lx, Ly, Lz of your model cuboid and the resolutions Nx, Ny, Nz.</li> <li>The "GeomFunc" you define at the end of the model file simply returns a 3D array containing the media definition for each voxel in the model cuboid. The media are referred to by a number, corresponding to the "j" defined in "mediaPropertiesFunc" at the end of the model file.</li> <li>You may optionally import your geometry from STL files as shown in example 18.</li> <li>After this step, when calling "plot(model,'G')", you will be shown a figure with the geometry you defined.</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">2. Calculate light distribution</h4><a id="user-content-2-calculate-light-distribution" class="anchor" aria-label="Permalink: 2. Calculate light distribution" href="#2-calculate-light-distribution"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>The section "%% Monte Carlo simulation" in the model file contains the definitions for the Monte Carlo simulation.</li> <li>After this step, when calling "plot(model,'MC')", you will be shown various figures; one with an overview of the optical properties, one with the absorbed light in the cuboid, one with the normalized fluence rate (NFR, roughly equivalent to normalized intensity or irradiance), and one showing the fluence rate at the cuboid boundaries (taking into account only the <em>exiting</em> photon packages, not the incident beam). The last figure will only be shown if some of your cuboid boundaries are "escaping" boundaries, i.e., boundary type 1 (all boundaries are escaping boundaries) or 2 (only the top is an escaping boundary).</li> <li>(Optional) If you set "model.MC.nExamplePaths" to an integer &gt; 0, you will also be shown a plot with the paths of the number of photons you requested.</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">3. (Optional) Include Fresnel reflection and refraction</h4><a id="user-content-3-optional-include-fresnel-reflection-and-refraction" class="anchor" aria-label="Permalink: 3. (Optional) Include Fresnel reflection and refraction" href="#3-optional-include-fresnel-reflection-and-refraction"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>Check out "Example3_RefractionReflection.m" and "Example17_CurvedRefractionReflection.m" on how to implement changing refractive indices in your model.</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">4. (Optional) Calculate fluorescence light distribution</h4><a id="user-content-4-optional-calculate-fluorescence-light-distribution" class="anchor" aria-label="Permalink: 4. (Optional) Calculate fluorescence light distribution" href="#4-optional-calculate-fluorescence-light-distribution"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>The section "%% Fluorescence Monte Carlo" contains the parameters for a fluorescence simulation, to be run after the distribution of excitation light has been calculated.</li> <li>To be able to run this step, your geometry definitions needs to include the fluorescence wavelength, "model.FMC.wavelength". Additionally, at least one of your media should be defined fluorescent, by defining its quantum yield <code>QY</code> in "mediaPropertiesFunc" at the end of your model file.</li> <li>After this step, when calling "plot(model,'FMC')", you will be shown the fluorescence emitter distribution, the fluorescent light fluence rate, the absorption within the cuboid, and the fluorescent light fluence rate at the cuboid boundaries.</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">5. (Optional) Simulate heat distribution</h4><a id="user-content-5-optional-simulate-heat-distribution" class="anchor" aria-label="Permalink: 5. (Optional) Simulate heat distribution" href="#5-optional-simulate-heat-distribution"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>In the "%% Heat simulation" section, you put the parameters for simulation of the temperature distribution, to be run after the Monte Carlo step(s)</li> <li>To simulate the heat diffusion, all media involved in the simulation must have the thermal properties volumetric heat capacity (VHC) and thermal conductivity (TC) defined in "mediaPropertiesFunc" at the end of your model file.</li> <li>If you want to model chemical changes such as tissue damage, the media that might undergo such change need to additionally have the Arrhenius activation energy (E) and the Arrhenius pre-exponential factor (A) defined.</li> <li>During the heat simulation, you will see an illustration of the temperature in your modelled cuboid.</li> <li>After this step, when calling "plot(model,'HS')", you will be shown various figures with the position of virtual temperature sensors in the cuboid, the temperature evolution at these positions, and whether there was some chemical change (based on the Arrhenius integral) in your cuboid.</li> <li>You can run multiple heat simulations defining different successive pulse trains as shown in "Example11_MultipleHeatSims.m"</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">6. (Optional) Imaging: Model the intensity distribution received by a detector/light collector</h4><a id="user-content-6-optional-imaging-model-the-intensity-distribution-received-by-a-detectorlight-collector" class="anchor" aria-label="Permalink: 6. (Optional) Imaging: Model the intensity distribution received by a detector/light collector" href="#6-optional-imaging-model-the-intensity-distribution-received-by-a-detectorlight-collector"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>Include a light collector for the incident light Monte Carlo, the fluorescence Monte Carlo, or for both. The light collector can either be a pixel array detector or a single pixel detector (such as a fibre). You can also optionally make your detector time-resolved.</li> <li>After running and calling either "plot(model,'MC')" or "plot(model,'FMC')", you will see an illustration of the geometry of your imaging system and the image of the scattered and/or fluorescence light.</li> <li>You can also choose to show the light impinging on the light collector in a time-resolved manner. Check out "Example6_TimeTagging.m" on how to do so.</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">7. (Optional) Calculate the far field angular distribution of light escaping the simulation volume</h4><a id="user-content-7-optional-calculate-the-far-field-angular-distribution-of-light-escaping-the-simulation-volume" class="anchor" aria-label="Permalink: 7. (Optional) Calculate the far field angular distribution of light escaping the simulation volume" href="#7-optional-calculate-the-far-field-angular-distribution-of-light-escaping-the-simulation-volume"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>See "Example7_FarField.m". Note that the far field does not include "killed" photons, that is, photons that have exited at a boundary where the refractive index is different to 1, or photons that exit on boundaries that are not "escaping".</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">8. (Optional) Use deposition criteria to show the normalized fluence rate array of only those photons which end up on the detector</h4><a id="user-content-8-optional-use-deposition-criteria-to-show-the-normalized-fluence-rate-array-of-only-those-photons-which-end-up-on-the-detector" class="anchor" aria-label="Permalink: 8. (Optional) Use deposition criteria to show the normalized fluence rate array of only those photons which end up on the detector" href="#8-optional-use-deposition-criteria-to-show-the-normalized-fluence-rate-array-of-only-those-photons-which-end-up-on-the-detector"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>See "Example8_CollectedFluenceRate.m".</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">9. (Optional) Programmatically assign values to the parameters</h4><a id="user-content-9-optional-programmatically-assign-values-to-the-parameters" class="anchor" aria-label="Permalink: 9. (Optional) Programmatically assign values to the parameters" href="#9-optional-programmatically-assign-values-to-the-parameters"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>See "Example9_GeometryParametricSweep.m" and "Example10_MediaPropertyParametricSweep.m" on how to implement sweeps of the parameters.</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">10. (Optional) Define fluence rate-, temperature- or fractional damage-dependent optical or thermal properties</h4><a id="user-content-10-optional-define-fluence-rate--temperature--or-fractional-damage-dependent-optical-or-thermal-properties" class="anchor" aria-label="Permalink: 10. (Optional) Define fluence rate-, temperature- or fractional damage-dependent optical or thermal properties" href="#10-optional-define-fluence-rate--temperature--or-fractional-damage-dependent-optical-or-thermal-properties"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>See Examples 12-15.</li> <li>By specifying the optical or thermal properties as a string (technically a char array) defining the formula as a function of fluence rate (FR), temperature (T) or fractional damage (FD), MCmatlab will take the dependence into account with an iterative approach.</li> </ul> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">11. (Optional) Enable CUDA GPU acceleration</h4><a id="user-content-11-optional-enable-cuda-gpu-acceleration" class="anchor" aria-label="Permalink: 11. (Optional) Enable CUDA GPU acceleration" href="#11-optional-enable-cuda-gpu-acceleration"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <ul dir="auto"> <li>See Example16_CUDAacceleration.m.</li> <li>If you have an Nvidia graphics card with compute capability at least 3.0, you can set useGPU = true to enable running on the GPU, greatly speeding up both the Monte Carlo and heat simulations.</li> </ul> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">List and explanation of input parameters</h3><a id="user-content-list-and-explanation-of-input-parameters" class="anchor" aria-label="Permalink: List and explanation of input parameters" href="#list-and-explanation-of-input-parameters"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">In the following we assume that the model object variable has been named "model". In principle, it could be given any name you want.</p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">Geometry parameters</h4><a id="user-content-geometry-parameters" class="anchor" aria-label="Permalink: Geometry parameters" href="#geometry-parameters"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto"><code>model.G.silentMode</code> [-] (Default: False) If true, MCmatlab will not make any command window text outputs during the geometry initialization.</p> <p dir="auto"><code>model.G.nx</code>, <code>model.G.ny</code>, <code>model.G.nz</code> [-] The number of bins in the x, y, and z direction, respectively. Higher numbers mean a more finely resolved result, but will also require much longer runtimes to reach a low noise level.</p> <p dir="auto"><code>model.G.Lx</code>, <code>model.G.Ly</code>, <code>model.G.Lz</code> [cm] The side lengths of the simulation cuboid, measured in cm.</p> <p dir="auto"><code>model.G.mediaPropertiesFunc</code> [-] A MATLAB function handle. This should be set to refer to the function at the end of the model file in which the media properties are defined. In principle you could have several different media property functions in your model file and the one referred to in this property is the one that MCmatlab uses, but in practice most model files will be built using only one media property function.</p> <p dir="auto"><code>model.G.mediaPropParams</code> [user-defined units] A user-defined cell array that you can use to contain all sorts of inputs you would like to use inside the mediaPropertiesFunc. This cell array is useful when doing parametric sweeps (many MC simulations in a for or while loop) in which the media properties vary.</p> <p dir="auto"><code>model.G.geomFunc</code> [-] (Similar to mediaPropertiesFunc above) A MATLAB function handle. This should be set to refer to the function at the end of the model file in which the model geometry is defined. In principle you could have several different geometry functions in your model file and the one referred to in this property is the one that MCmatlab uses, but in practice most model files will be built using only one geometry function.</p> <p dir="auto"><code>model.G.geomFuncParams</code> [user-defined units] (Similar to mediaPropParams above) A user-defined cell array that you can use to contain all sorts of inputs you would like to use inside the geomFunc. This cell array is useful when doing parametric sweeps (many MC simulations in a for or while loop) in which the geometry varies.</p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">(Excitation) Monte Carlo parameters</h4><a id="user-content-excitation-monte-carlo-parameters" class="anchor" aria-label="Permalink: (Excitation) Monte Carlo parameters" href="#excitation-monte-carlo-parameters"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto"><code>model.MC.useGPU</code> [-] (Default: False) If true, will run the MC simulation on GPU. If false, will use CPU.</p> <p dir="auto"><code>model.MC.GPUdevice</code> [-] (Default: 0) The GPU device to use for GPU accelerated computations. 0 corresponds to the first device. For systems with multiple GPUs, you can launch simulations to different GPUs by varying this property and with the use of, e.g., a MATLAB parallel-for (parfor) loop.</p> <p dir="auto"><code>model.MC.simulationTimeRequested</code> [minutes] (Mutually exclusive with model.MC.nPhotonsRequested) The time to run the MC simualtion for, in minutes. The number of photos launched will vary from run to run.</p> <p dir="auto"><code>model.MC.nPhotonsRequested</code> [-] (Mutually exclusive with model.MC.simulationTimeRequested) The number of photons to launch. The execution time will vary from run to run.</p> <p dir="auto">`model.MC.requestCollectedPhotons [-] (Default: False) (Only used if model.MC.nPhotonsRequested is specified) If true, model.MC.nPhotonsRequested is interpreted as the requested number of collected photon packets, rather than launched photon packets.</p> <p dir="auto"><code>model.MC.silentMode</code> [-] (Default: False) If true, MCmatlab will not make any command window text outputs during the MC simulation.</p> <p dir="auto"><code>model.MC.useAllCPUs</code> [-] (Default: False) (Has no effect on MacOS or if model.MC.useGPU = true) If true, MCmatlab will launch a number of threads equal to the number of CPU logical processors on the system. This will lead to the fastest execution but may make the system slow to respond to user inputs (mouse clicks etc.) for the duration of the simulation. If false, MCmatlab will still be multithreaded but will leave one CPU logical processor unused. This will yield almost the same speed of execution but will make the system more responsive while the simulation is running.</p> <p dir="auto"><code>model.MC.calcNFR</code> [-] (Default: True) If true, will calculate and store the normalized fluence rate (NFR) 3D or 4D array (4D if simulating broadband light). The array takes 8*nx*ny*nz*nl bytes of memory (and disk space, if the resulting model file is saved to disk subsequently) For some simulations in which you are only interested, for example, in the detector image/power, you might not need the NFR and could therefore set this to false.</p> <p dir="auto"><code>model.MC.nExamplePaths</code> [-] (Default: 0) If set to a positive integer N, will store the paths of the first N photons for subsequent visualization during the plotting. This is useful to visualize how the photons move around the cuboid.</p> <p dir="auto"><code>model.MC.farFieldRes</code> [pixels] (Default: 0) If set to a positive integer N, MCmatlab will calculate the far field direction angles of the escaping photons and store them in a 2D NxN array (theta,phi on the unit sphere) for later visualization.</p> <p dir="auto"><code>model.MC.matchedInterfaces</code> [-] (Default: True) If true, will set all refractive indices to 1, disregarding any refractive indices specified in the media properties function. In this case, no Fresnel reflection and refraction will be simulated.</p> <p dir="auto"><code>model.MC.smoothingLengthScale</code> [cm] (Only used if matchedInterfaces = false) The characteristic length scale to use for smoothing of the Sobel filter applied to the normal vectors of the non-matched interfaces within the geometry. See <a href="https://www.spiedigitallibrary.org/journals/journal-of-biomedical-optics/volume-25/issue-02/025001/Modeling-voxel-based-Monte-Carlo-light-transport-with-curved-and/10.1117/1.JBO.25.2.025001.full" rel="nofollow">https://www.spiedigitallibrary.org/journals/journal-of-biomedical-optics/volume-25/issue-02/025001/Modeling-voxel-based-Monte-Carlo-light-transport-with-curved-and/10.1117/1.JBO.25.2.025001.full</a> for a description of the technique used. The use of such smoothing enables simulation of reflection and refraction even on oblique interfaces, despite the geometry being defined on a rectangular cuboid mesh. See Example17_CurvedRefractionReflection.m.</p> <p dir="auto"><code>model.MC.boundaryType</code> [-] 0: No escaping boundaries 1: All cuboid boundaries are escaping 2: Top cuboid boundary only is escaping 3: Top and bottom boundaries are escaping, while the side boundaries are cyclic Photons that hit a boundary that is "escaping" and where the refractive index is equal to 1 will be considered an "escaped" photon, and may, depending on the position and direction, be registered by the detector/light collector. When a photon encounters a boundary that is not escaping, it is allowed to propagate beyond the edge up to a distance of 2½ times the value of (Lx or Ly or Lz) before the photon is finally killed and no longer simulated. Allowing photons to propagate beyond the cuboid boundaries enable the photons to potentially scatter back into the simulation volume. The more boundaries are escaping, the faster the simulation will run because fewer photons outside the cuboid have to be simulated. When a photon hits a cyclic boundary, it will exit and immediately enter the cuboid again on the opposite boundary, as if the cuboid is periodic. In other words, if your geometry and light source is periodically repeating in x and y (such as a simple layered model illuminated by an infinite plane wave), you need only simulate just one unit cell of this pattern and use cyclic x and y boundaries.</p> <p dir="auto"><code>model.MC.wavelength</code> [nm] The wavelength(s) of the light. May be scalar or 1D array. Media properties in the mediaPropertiesFunc may be dependent on the wavelength of the light. The wavelength does not actually change anything in the MC simulation itself aside from the change in the media properties. Wavelength is also used to calculate the fluorescence emission powers based on the quantum yields of the fluorescers. If wavelength is specified as a 1D array, broadband simulations will be performed.</p> <p dir="auto"><code>model.MC.lightSource.sourceType</code> [-] (Note that lightSource can be abbreviated LS in your code) 0: Pencil beam A pencil beam is a beam with zero width and zero divergence. 1: Isotropically emitting line or point source This option is the only one in which the light will originate from within the cuboid. All other options have photons packets starting at the top surface, z = 0. 2: Infinite plane wave A beam with infinite width, but zero divergence. 3: Laguerre-Gaussian LG01 beam A ray-based emulation of the donut-shaped Laguerre-Gaussian LG01 beam. 4: Radial-factorizable beam A beam in which the focus beam profile can be written as I(x,y) = Ir(r), where r = sqrt(x^2+y^2), and similarly for the angular distribution. Circular Gaussian beams can be written in this form. 5: X/Y factorizable beam A beam in which the focus beam profile can be written as I(x,y) = Ix(x)*Iy(y), and similarly for the angular distribution. Rectangular LED emitters can be written in this way, as well as Gaussian (circular and elliptical) beams.</p> <p dir="auto"><code>model.MC.lightSource.emitterLength</code> [cm] (Only used for model.MC.lightSource.sourceType = 1. Default: 0) The length of the line emitter. If zero, the emitter is a point source.</p> <p dir="auto"><code>model.MC.lightSource.focalPlaneIntensityDistribution.radialDistr</code> [-] (Note that focalPlaneIntensityDistribution can be abbreviated FPID in your code) (Only used for sourceType = 4) Radial intensity distribution in the focal plane. 0: Top-hat 1: Gaussian Array: Custom. Doesn't need to be normalized.</p> <p dir="auto"><code>model.MC.lightSource.focalPlaneIntensityDistribution.radialWidth</code> [cm] (Note that focalPlaneIntensityDistribution can be abbreviated FPID in your code) (Only used for sourceType = 4) Radial width of the intensity distribution in the focal plane. If FPID.radialDistr is set to 0 or 1, this is the 1/e^2 radius If FPID.radialDistr is set to an array, this is the half-width of the full distribution</p> <p dir="auto"><code>model.MC.lightSource.focalPlaneIntensityDistribution.XDistr</code>, <code>model.MC.lightSource.focalPlaneIntensityDistribution.YDistr</code> [-] (Note that focalPlaneIntensityDistribution can be abbreviated FPID in your code) (Only used for sourceType = 5) X and Y distribution of the intensity in the focal plane. 0: Top-hat 1: Gaussian Array: Custom. Doesn't need to be normalized.</p> <p dir="auto"><code>model.MC.lightSource.focalPlaneIntensityDistribution.XWidth</code>, <code>model.MC.lightSource.focalPlaneIntensityDistribution.YWidth</code> [cm] (Note that focalPlaneIntensityDistribution can be abbreviated FPID in your code) (Only used for sourceType = 5) X and Y width of the intensity distribution in the focal plane. If FPID.XDistr/FPID.YDistr is set to 0 or 1, this is the 1/e^2 radius If FPID.XDistr/FPID.YDistr is set to an array, this is the half-width of the full distribution</p> <p dir="auto"><code>model.MC.lightSource.angularIntensityDistribution.radialDistr</code> [-] (Note that angularIntensityDistribution can be abbreviated AID in your code) (Only used for sourceType = 4) Radial distribution of the angular intensity. 0: Top-hat 1: Gaussian 2: Cosine (Lambertian) Array: Custom. Doesn't need to be normalized.</p> <p dir="auto"><code>model.MC.lightSource.angularIntensityDistribution.radialWidth</code> [rad] (Note that angularIntensityDistribution can be abbreviated AID in your code) (Only used for sourceType = 4 and if AID.radialDistr is not 2) Radial width of the angular intensity distribution. If AID.radialDistr is set to 0 or 1, this is the 1/e^2 half-angle. If AID.radialDistr is set to an array, this is the half-angle of the full distribution. For a diffraction limited Gaussian beam, this should be set to model.MC.wavelength*1e-9/(pi*model.MC.lightSource.focalPlaneIntensityDistribution.radialWidth*1e-2))</p> <p dir="auto"><code>model.MC.lightSource.angularIntensityDistribution.XDistr</code>, <code>model.MC.lightSource.angularIntensityDistribution.YDistr</code> [-] (Note that angularIntensityDistribution can be abbreviated AID in your code) (Only used for sourceType = 5) X and Y distribution of the angular intensity. 0: Top-hat 1: Gaussian 2: Cosine (Lambertian) Array: Custom. Doesn't need to be normalized.</p> <p dir="auto"><code>model.MC.lightSource.angularIntensityDistribution.XWidth</code>, <code>model.MC.lightSource.angularIntensityDistribution.YWidth</code> [rad] (Note that angularIntensityDistribution can be abbreviated AID in your code) (Only used for sourceType = 5 and if AID.XDistr or AID.YDistr is not 2) Radial width of the angular intensity distribution. If AID.XDistr/AID.YDistr is set to 0 or 1, this is the 1/e^2 half-angle. If AID.XDistr/AID.YDistr is set to an array, this is the half-angle of the full distribution.</p> <p dir="auto"><code>model.MC.lightSource.xFocus</code>, <code>model.MC.lightSource.yFocus</code>, <code>model.MC.lightSource.zFocus</code> [cm] The focus (or source) position x,y,z coordinates.</p> <p dir="auto"><code>model.MC.lightSource.psi</code> [rad] (Only used for sourceType = 5. Default: 0) Axial rotation angle of the beam.</p> <p dir="auto"><code>model.MC.lightSource.theta</code>, <code>model.MC.lightSource.phi</code> [rad] Polar and azimuthal angle of the beam center axis.</p> <p dir="auto"><code>model.MC.sourceDistribution</code> [-] If set to an array of dimensions [nx, ny, nz, nLambda], this will be interpreted as the spatial and spectral distribution of emitters. If this is specified, the contents of lightSource will be disregarded. This array will be normalized by MCmatlab during the call to runMonteCarlo().</p> <p dir="auto"><code>model.MC.depositionCriteria.minScatterings</code>, <code>model.MC.depositionCriteria.maxScatterings</code>, <code>model.MC.depositionCriteria.minRefractions</code>, <code>model.MC.depositionCriteria.maxRefractions</code>, <code>model.MC.depositionCriteria.minReflections</code>, <code>model.MC.depositionCriteria.maxReflections</code>, <code>model.MC.depositionCriteria.minInterfaceTransitions</code>, <code>model.MC.depositionCriteria.maxInterfaceTransitions</code> [-] The minimum and maximum number of scattering, refraction, reflection and interface transition events the photon packet must have undergone in order to be registered as an example photon path and to deposit weight into the output arrays (normalized fluence rate, normalized boundary irradiances, image and far field). There is an implied AND between all the criteria. Note that the underlying absorption and propagation of all photon packets are independent of the specified deposition criteria.</p> <p dir="auto"><code>model.MC.depositionCriteria.minMediumIdxToConsider</code>, <code>model.MC.depositionCriteria.maxMediumIdxToConsider</code> [-] The minimum and maximum medium index that the above deposition criteria apply to. For example, if you've specified minScatterings = 2, minMediumIdxToConsider = 4 and maxMediumIdxToConsider = 5, then only photons that have experienced at least 2 scattering events in media 4 and/or 5 will deposit their weight in the output arrays and register as photon paths. It doesn't matter how many scattering events have happened in other media.</p> <p dir="auto">Interface transitions and refractions will be considered if the medium transitioned <em>into</em> has index between minMediumIdxToConsider and maxMediumIdxToConsider.</p> <p dir="auto">Keep in mind that you can rearrange the media in the media definition and geometry function as required so that the indices of the set of media that you want to consider in deposition criteria are in a contiguous interval.</p> <p dir="auto"><code>model.MC.depositionCriteria.evaluateOnlyAtEndOfLife</code> [-] If evaluateOnlyAtEndOfLife is false, the photons will only deposit weight into the output arrays and register as photon paths in those segments of the paths where the criteria are satisfied. If it is true, weight is deposited and path is registered along the full path if the criteria are satisfied at the end of the photon's life span.</p> <p dir="auto"><code>model.MC.depositionCriteria.onlyCollected</code> [-] If evaluateOnlyAtEndOfLife is true, you may also specify onlyCollected. It is an extra criterion that states that the photon must have been collected on the light collector.</p> <p dir="auto"><code>model.MC.P</code> [W] (Default: 1) (Only used for the thermal simulations and for any Monte Carlo simulations in which the optical or thermal parameters depend on the fluence rate (FR), fractional damage (FD) or temperature (T)) Incident pulse peak power. In case of infinite plane waves, this is only the power incident upon the cuboid's top surface.</p> <p dir="auto"><code>model.MC.spectrumFunc</code> [-] (Default: 1) (Only used for broadband simulations) A function handle that takes wavelength as an input and returns the spectral power of the source as an output. This function doesn't need to be normalized, as the total power emitted across all simulated wavelengths will be normalized to <code>model.MC.P</code> regardless.</p> <p dir="auto"><code>model.MC.FRinitial</code> [W/cm^2] (Only used for MC simulations in which the optical properties depend on the fluence rate (FR)) Initial guess for the fluence rate distribution in, to be used for iterative fluence rate dependent simulations.</p> <p dir="auto"><code>model.MC.FRdepIterations</code> [-] (Only used for MC simulations in which the optical properties depend on the fluence rate (FR)) The number of iterations (times the MC simulation needs to be run) each time a new calculation of the MC outputs is requested. Test for yourself how high this number needs to be for your model. In my tests, 20 was enough.</p> <p dir="auto"><code>model.MC.useLightCollector</code> [-] (Default: False) A logical (boolean) to specify whether the MC simulation should keep track of whether photons hit the light collector/detector.</p> <p dir="auto">(The following LC properties are only used if useLightCollector = true)</p> <p dir="auto"><code>model.MC.lightCollector.f</code> [cm] (Note that lightCollector can be abbreviated LC in your code) If the light collector is supposed to be an objective lens, this is its focal length. If the light collector is supposed to be a fiber tip this should be set to Inf (infinity)</p> <p dir="auto"><code>model.MC.lightCollector.x</code>, <code>model.MC.lightCollector.y</code>, <code>model.MC.lightCollector.z</code> [cm] (Note that lightCollector can be abbreviated LC in your code) If model.MC.lightCollector.f is finite (light collector is an objective lens), this is the x, y, z position of the center of the focal plane of the objective lens. If model.MC.lightCollector.f is infinite (light collector is a fiber tip), this is the x, y, z position of the center of the fiber tip.</p> <p dir="auto"><code>model.MC.lightCollector.theta</code>, <code>model.MC.lightCollector.phi</code> [rad] (Note that lightCollector can be abbreviated LC in your code) Polar and azimuthal angle of direction that the light collector is facing</p> <p dir="auto"><code>model.MC.lightCollector.NA</code> [-] (Note that lightCollector can be abbreviated LC in your code) (Only used for infinite f) Fiber numerical aperture.</p> <p dir="auto"><code>model.MC.lightCollector.diam</code> [cm] (Note that lightCollector can be abbreviated LC in your code) Diameter of the light collector aperture. For an ideal thin lens with numerical aperture NA, this is 2f*tan(asin(NA)).</p> <p dir="auto"><code>model.MC.lightCollector.fieldSize</code> [cm] (Note that lightCollector can be abbreviated LC in your code) (Only used for finite f) Field size of the imaging system, that is, the diameter of area in object plane that gets imaged.</p> <p dir="auto"><code>model.MC.lightCollector.res</code> [pixels] (Note that lightCollector can be abbreviated LC in your code) (Only used for finite f) X and Y resolution of light collector, only used for finite f</p> <p dir="auto"><code>model.MC.lightCollector.tStart</code>, <code>model.MC.lightCollector.tEnd</code> [s] (Note that lightCollector can be abbreviated LC in your code) Start and end time of the detection time-of-flight interval. Note that photons arriving before tStart will still be registered but all binned together in a single bin containing all "too-early" photons. Likewise, all photons arriving after tEnd are binned into a "too-late" bin.</p> <p dir="auto"><code>model.MC.lightCollector.nTimeBins</code> [-] (Note that lightCollector can be abbreviated LC in your code) (Default: 0) Number of bins between tStart and tEnd. If zero, the measurement is not time-resolved.</p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">Fluorescence Monte Carlo parameters</h4><a id="user-content-fluorescence-monte-carlo-parameters" class="anchor" aria-label="Permalink: Fluorescence Monte Carlo parameters" href="#fluorescence-monte-carlo-parameters"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">The following properties exist for fluorescence Monte Carlo simulations, and they work the same as for regular MC simulations: <code>FMC.useGPU</code>, <code>FMC.GPUdevice</code>, <code>FMC.simulationTimeRequested</code>, <code>FMC.nPhotonsRequested</code>, <code>FMC.silentMode</code>, <code>FMC.useAllCPUs</code>, <code>FMC.calcNormalizedFluenceRate</code>, <code>FMC.nExamplePaths</code>, <code>FMC.farFieldRes</code>, <code>FMC.matchedInterfaces</code>, <code>FMC.smoothingLengthScale</code>, <code>FMC.boundaryType</code>, <code>FMC.wavelength</code>, <code>FMC.useLightCollector</code>, <code>FMC.lightCollector.x</code>, <code>FMC.lightCollector.y</code>, <code>FMC.lightCollector.z</code>, <code>FMC.lightCollector.theta</code>, <code>FMC.lightCollector.phi</code>, <code>FMC.lightCollector.f</code>, <code>FMC.lightCollector.diam</code>, <code>FMC.lightCollector.fieldSize</code>, <code>FMC.lightCollector.NA</code>, <code>FMC.lightCollector.res</code></p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">Heat solver parameters</h4><a id="user-content-heat-solver-parameters" class="anchor" aria-label="Permalink: Heat solver parameters" href="#heat-solver-parameters"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto"><code>model.HS.useGPU</code> [-] (Default: false) Use CUDA acceleration for the heat simulation solver for NVIDIA GPUs</p> <p dir="auto"><code>model.HS.silentMode</code> [-] (Default: false) If true, MCmatlab will not make any command window text outputs during the heat simulation.</p> <p dir="auto"><code>model.HS.useAllCPUs</code> [-] (Default: false) (Has no effect on MacOS or if model.MC.useGPU = true) If true, MCmatlab will launch a number of threads equal to the number of CPU logical processors on the system. This will lead to the fastest execution but may make the system slow to respond to user inputs (mouse clicks etc.) for the duration of the simulation. If false, MCmatlab will launch will still be multithreaded but will leave one CPU logical processor unused. This will yield almost the same speed of execution but will make the system more responsive while the simulation is running.</p> <p dir="auto"><code>model.HS.makeMovie</code> [-] (Default: false) (Only used if silentMode = false) If true, MCmatlab will record each frame of the volumetric temperature plot and get ready to save the frames to a movie file.</p> <p dir="auto"><code>model.HS.deferMovieWrite</code> [-] (Default: false) (Only used if silentMode = false and makeMovie = true) If false, MCmatlab will save the recorded frames to a movie file. If true, the frames are still stored within the model object so that subsequent heat simulations can be concatenated to them before saving.</p> <p dir="auto"><code>model.HS.largeTimeSteps</code> [-] (Default: false) If true, calculations will be faster, but some voxel temperatures may be slightly less precise. Test for yourself whether this precision is acceptable for your application.</p> <p dir="auto"><code>model.HS.heatBoundaryType</code> [-] The type of boundary condition to use for the heat solver. 0: Insulating boundaries 1: Constant-temperature boundaries (heat-sinked)</p> <p dir="auto"><code>model.HS.nPulses</code> [-] Number of consecutive pulses, each with an illumination phase and a diffusion phase. If simulating only illumination or only diffusion, use nPulses = 1.</p> <p dir="auto"><code>model.HS.durationOn</code>, <code>model.HS.durationOff</code> [s] Pulse on-duration and off-duration</p> <p dir="auto"><code>model.HS.durationEnd</code> [s] Non-illuminated relaxation time to add to the end of the simulation to let temperature diffuse after the pulse train.</p> <p dir="auto"><code>model.HS.T</code> [deg C] (Functions both as an input and an output property) Initial and final temperature, can be scalar or 3D array of dimensions nx, ny, nz.</p> <p dir="auto"><code>model.HS.plotTempLimits</code> [deg C] An array of two values designating the expected range of temperatures, used only for setting the color scale in the plot. One or both values can be NaN to let the limit be set to the minimum or maximum of the data. For example [NaN 100] means the lower color limit is automatically set to the minimum value in the data, but the upper color limit is fixed at 100.</p> <p dir="auto"><code>model.HS.nUpdates</code> [-] Number of times data is extracted for plots during each pulse. A minimum of 1 update is performed in each phase (2 for each pulse consisting of an illumination phase and a diffusion phase)</p> <p dir="auto"><code>model.HS.mediaPropRecalcPeriod</code> [-] (Used only if optical or thermal parameters have been specified to be dependent on temperature (T)) Every time this many updates have passed, the media properties will be recalculated (including, if needed, re-running MC and FMC steps). Check that this is low enough to ensure convergence of your results.</p> <p dir="auto"><code>model.HS.slicePositions</code> [-] (Default: [0.5 1 1]) An array of three values, describing the fractional x, y, z positions on a scale from 0 to 1 to place the volumetric slices at.</p> <p dir="auto"><code>model.HS.tempSensorPositions</code> [cm] (Default: empty array) A 2D array with three columns. Each row describes the x, y, z coordinates of a temperature sensor placed within the cuboid, at which the temperature will be recorded for subsequent plotting as a function of time. Leave the matrix empty ([]) to disable temperature sensors.</p> <div class="markdown-heading" dir="auto"><h3 tabindex="-1" class="heading-element" dir="auto">List and explanation of output properties</h3><a id="user-content-list-and-explanation-of-output-properties" class="anchor" aria-label="Permalink: List and explanation of output properties" href="#list-and-explanation-of-output-properties"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">As in the previous section, we assume that the model object variable has been named "model". In principle, it could be given any name you want.</p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">Geometry properties</h4><a id="user-content-geometry-properties" class="anchor" aria-label="Permalink: Geometry properties" href="#geometry-properties"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto"><code>model.G.dx</code>, <code>model.G.dy</code>, <code>model.G.dz</code> [cm] The side lengths of the voxels. They are simply calculated as the side length of the simulation cuboid divided by the number of bins, for example, model.G.Lx/model.G.nx.</p> <p dir="auto"><code>model.G.x</code>, <code>model.G.y</code>, <code>model.G.z</code> [cm] 1D arrays with the x, y or z coordinate values corresponding to the centers of the voxels You can use these for easy plotting of slices, see for example the entry on NFR in the MC section below.</p> <p dir="auto"><code>model.G.M_raw</code> [-] 3D (xyz) array in coordinate order of the tissue indices as calculated from the geomFunc. This is the array that is plotted in the figure called Geometry Illustration.</p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">(Excitation) Monte Carlo properties</h4><a id="user-content-excitation-monte-carlo-properties" class="anchor" aria-label="Permalink: (Excitation) Monte Carlo properties" href="#excitation-monte-carlo-properties"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto"><code>model.MC.simulationTime</code> [min] The actual simulation time of the most recent Monte Carlo simulation run. If you did not define model.MC.nPhotonsRequested, then the simulation is timed and model.MC.simulationTime should be very close to `model.MC.simulationTimeRequested.</p> <p dir="auto"><code>model.MC.nPhotons</code> [-] The actual number of photon packets launched in the most recent Monte Carlo simulation run. If you defined model.MC.nPhotonsRequested, then model.MC.nPhotons will be equal to that number.</p> <p dir="auto"><code>model.MC.nPhotonsCollected</code> [-] The actual number of photon packets that was registered on the light collected in the most recent Monte Carlo simulation run. If you set model.MC.requestCollectedPhotons = true, then model.MC.nPhotonsCollected will be equal to model.MC.nPhotonsRequested.</p> <p dir="auto"><code>model.MC.mediaProperties</code> [-] A struct that contains the media properties as evaluated at the specified excitation Monte Carlo wavelength, model.MC.wavelength.</p> <p dir="auto"><code>model.MC.M</code> [-] A 3D (xyz) array. If the media properties do not contain dependences on fluence rate (FR), temperature (T) or fractional damage (FD), then this array will simply be equal to model.G.M_raw. Otherwise, model.MC.M will be the "split" version of model.G.M_raw, in which those media that have dependences have been split into the specified number of sub-media with different optical/thermal properties for the purposes of the simulations.</p> <p dir="auto"><code>model.MC.interfaceNormals</code> [-] A 2D array of dimension (2 x (nx<em>ny</em>nz)) where local interface normal vector angles are stored. Each column contains the theta, phi angles for one voxel's interface normal vector. Used for calculated of refraction and reflection on oblique and curved interfaces between media with different refractive index.</p> <p dir="auto"><code>model.MC.examplePaths</code> [cm] and [-] A 2D array which stores the example paths' coordinates and remaining weight. Each column is a data point where the first three rows are the x, y, z position of the photon packet and the fourth row is the remaining weight (energy) of the photon packet. Different photon trajectories are separated by a column of NaNs.</p> <p dir="auto"><code>model.MC.normalizedFluenceRate</code> [W/cm^2/W.incident] (Note that normalizedFluenceRate can be abbreviated NFR in your code) A 3D or 4D array (4D if simulating broadband light) (x,y,z,lambda) of normalized fluence rate values. This is what's plotted in figure 4. If you want to plot a slice out of this distribution, you could for example do it with these three lines of code:</p> <ul dir="auto"> <li><code>NFRslice = squeeze(model.MC.NFR(51,:,:));</code> Extracts the slice corresponding to the 51st x value. <code>squeeze</code> is to remove the x singleton dimension, giving you a 2D (yz) array of normalized fluence rates.</li> <li><code>figure(100);</code></li> <li><code>imagesc(model.G.y,model.G.z,NFRslice.');</code> We can use the 1D coordinate arrays from model.G for the y and z coordinate values. The <code>.'</code> is there because Mathworks has designed the imagesc function to plot the first coordinate along the vertical axis and the second coordinate along the horizontal axis, which is the opposite of what we want.</li> </ul> <p dir="auto"><code>model.MC.normalizedAbsorption</code> [W/cm^3/W.incident] (Note that normalizedAbsorption can be abbreviated NA in your code) A 3D or 4D array (4D if simulating broadband light) (x,y,z,lambda) of normalized absorption values. This is what's plotted in figure 3.</p> <p dir="auto"><code>model.MC.farField</code> [W/sr/W.incident] A 2D or 3D (theta,phi,lambda) array of normalized radiant intensity values for the light that escaped the simulation cuboid. The axes are the polar and azimuthal angles, described below.</p> <p dir="auto"><code>model.MC.farFieldTheta</code> [rad] A 1D array of polar angles corresponding to the first dimension of model.MC.farField.</p> <p dir="auto"><code>model.MC.farFieldPhi</code> [rad] A 1D array of azimuthal angles corresponding to the second dimension of model.MC.farField.</p> <p dir="auto"><code>model.MC.normalizedIrradiance_xpos</code>, <code>model.MC.normalizedIrradiance_xneg</code>, <code>model.MC.normalizedIrradiance_ypos</code>, <code>model.MC.normalizedIrradiance_yneg</code>, <code>model.MC.normalizedIrradiance_zpos</code>, <code>model.MC.normalizedIrradiance_zneg</code> [W/cm^2/W.incident] (Note that normalizedIrradiance can be abbreviated NI in your code) 2D or 3D (xy, xz or yz - with lambda as third dimension) arrays of normalized irradiances of the light hitting the boundaries (either escaping or killed). For example, the property named <code>model.MC.NI_xpos</code> designates the light that hits the surface that is orthogonal to the x axis and placed on the positive x side, whereas the <code>model.MC.NI_xneg</code> refers to the surface orthogonal to the x axis and placed on the negative x side. model.MC.boundaryType determine which of these arrays are calculated. <code>model.MC.NI_zneg</code> is of special interest to users interested in calculating the reflectance, which can be found as the integral over the array:</p> <ul dir="auto"> <li><code>R = model.G.dx*model.G.dy*sum(model.MC.NI_zneg(:));</code></li> </ul> <p dir="auto"><code>model.MC.lightCollector.image</code> [W/cm^2/W.incident] If <code>model.MC.lightCollector.res == 1</code>, this is a scalar or 1D array with the normalized power registered on the light collector as function of wavelength. If <code>model.MC.lightCollector.res &gt; 1</code>, this is a 2D or 3D array (X,Y,lambda) of normalized irradiances registered on the light collector. This array describes the light distribution you would get on a camera looking at the cuboid through an objective lens.</p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">Fluorescence Monte Carlo properties</h4><a id="user-content-fluorescence-monte-carlo-properties" class="anchor" aria-label="Permalink: Fluorescence Monte Carlo properties" href="#fluorescence-monte-carlo-properties"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">All the output properties described above for excitation Monte Carlo are also provided for fluorescence Monte Carlo in the model.FMC object.</p> <div class="markdown-heading" dir="auto"><h4 tabindex="-1" class="heading-element" dir="auto">Heat solver properties</h4><a id="user-content-heat-solver-properties" class="anchor" aria-label="Permalink: Heat solver properties" href="#heat-solver-properties"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto"><code>model.HS.M</code> [-] A 3D (xyz) array. If the media properties do not contain dependences on fluence rate (FR), temperature (T) or fractional damage (FD), then this array will simply be equal to model.G.M_raw. Otherwise, model.HS.M will be the "split" version of model.G.M_raw, in which those media that have dependences have been split into the specified number of sub-media with different optical/thermal properties for the purposes of the simulations.</p> <p dir="auto"><code>model.HS.T</code> [deg C] A 3D (xyz) array with the final temperature values of the simulation.</p> <p dir="auto"><code>model.HS.Omega</code> [-] A 3D (xyz) array with the final Omega values of the simulation. Omega describes the thermally induced tissue damage calculated according to the Arrhenius damage integral.</p> <p dir="auto"><code>model.HS.maxMediaTemps</code> [deg C] A 1D array that contains the maximal temperatures obtained in each tissue type involved in the simulation.</p> <p dir="auto"><code>model.HS.sensorsTimeVector</code> [s] A 1D array of time values that should be used for plotting the sensorTemps data (see below).</p> <p dir="auto"><code>model.HS.sensorTemps</code> [deg C] A 2D array of temperatures measured at the specified sensor positions. Each row corresponds to one sensor. Use the model.HS.sensorsTimeVector as the time values when plotting this data.</p> <div class="markdown-heading" dir="auto"><h2 tabindex="-1" class="heading-element" dir="auto">Contribution guidelines</h2><a id="user-content-contribution-guidelines" class="anchor" aria-label="Permalink: Contribution guidelines" href="#contribution-guidelines"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p dir="auto">You are very welcome to clone the repository and add features of your own. If you want to report a bug or are missing a feature, shoot me an email, see below.</p> <div class="markdown-heading" dir="auto"><h2 tabindex="-1" class="heading-element" dir="auto">Who do I talk to?</h2><a id="user-content-who-do-i-talk-to" class="anchor" aria-label="Permalink: Who do I talk to?" href="#who-do-i-talk-to"><svg class="octicon octicon-link" viewBox="0 0 16 16" version="1.1" width="16" height="16" aria-hidden="true"><path d="m7.775 3.275 1.25-1.25a3.5 3.5 0 1 1 4.95 4.95l-2.5 2.5a3.5 3.5 0 0 1-4.95 0 .751.751 0 0 1 .018-1.042.751.751 0 0 1 1.042-.018 1.998 1.998 0 0 0 2.83 0l2.5-2.5a2.002 2.002 0 0 0-2.83-2.83l-1.25 1.25a.751.751 0 0 1-1.042-.018.751.751 0 0 1-.018-1.042Zm-4.69 9.64a1.998 1.998 0 0 0 2.83 0l1.25-1.25a.751.751 0 0 1 1.042.018.751.751 0 0 1 .018 1.042l-1.25 1.25a3.5 3.5 0 1 1-4.95-4.95l2.5-2.5a3.5 3.5 0 0 1 4.95 0 .751.751 0 0 1-.018 1.042.751.751 0 0 1-1.042.018 1.998 1.998 0 0 0-2.83 0l-2.5 2.5a1.998 1.998 0 0 0 0 2.83Z"></path></svg></a></div> <p 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