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</div> <div class="control"> <button class="button is-small is-link">Go</button> </div> </div> </form> </div> </div> <ol class="breathe-horizontal" start="1"> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1701.00164">arXiv:1701.00164</a> <span> [<a href="https://arxiv.org/pdf/1701.00164">pdf</a>, <a href="https://arxiv.org/format/1701.00164">other</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="High Energy Astrophysical Phenomena">astro-ph.HE</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Instrumentation and Methods for Astrophysics">astro-ph.IM</span> </div> </div> <p class="title is-5 mathjax"> Effect of pressure and temperature corrections on muon flux variability at ground level and underground </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Savic%2C+M">Mihailo Savic</a>, <a href="/search/physics?searchtype=author&query=Dragic%2C+A">Aleksandar Dragic</a>, <a href="/search/physics?searchtype=author&query=Veselinovic%2C+N">Nikola Veselinovic</a>, <a href="/search/physics?searchtype=author&query=Udovicic%2C+V">Vladimir Udovicic</a>, <a href="/search/physics?searchtype=author&query=Banjanac%2C+R">Radomir Banjanac</a>, <a href="/search/physics?searchtype=author&query=Jokovic%2C+D">Dejan Jokovic</a>, <a href="/search/physics?searchtype=author&query=Maletic%2C+D">Dimitrije Maletic</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1701.00164v1-abstract-short" style="display: inline;"> In Low Background Laboratory at Institute of Physics Belgrade, plastic scintillators are used to continuously monitor flux of the muon component of secondary cosmic rays. Measurements are performed on the surface as well as underground (25 m.w.e depth). Temperature effect on muon component of secondary cosmic rays is well known and several methods to correct for it are already developed and widely… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1701.00164v1-abstract-full').style.display = 'inline'; document.getElementById('1701.00164v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1701.00164v1-abstract-full" style="display: none;"> In Low Background Laboratory at Institute of Physics Belgrade, plastic scintillators are used to continuously monitor flux of the muon component of secondary cosmic rays. Measurements are performed on the surface as well as underground (25 m.w.e depth). Temperature effect on muon component of secondary cosmic rays is well known and several methods to correct for it are already developed and widely used. Here, we apply integral method to calculate correction coefficients and use GFS (Global Forecast System) model to obtain atmospheric temperature profiles. Atmospheric corrections reduce variance of muon flux and lead to improved sensitivity to transient cosmic ray variations. Influence of corrections on correlation with neutron monitor data is discussed. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1701.00164v1-abstract-full').style.display = 'none'; document.getElementById('1701.00164v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 31 December, 2016; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> January 2017. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">XXV ECRS 2016 Proceedings - eConf C16-09-04.3</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1305.2572">arXiv:1305.2572</a> <span> [<a href="https://arxiv.org/pdf/1305.2572">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.1016/j.nima.2014.01.065">10.1016/j.nima.2014.01.065 <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> On the omnipresent background gamma radiation of the continuous spectrum </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Banjanac%2C+R">R. Banjanac</a>, <a href="/search/physics?searchtype=author&query=Maleti%C4%87%2C+D">D. Maleti膰</a>, <a href="/search/physics?searchtype=author&query=Jokovi%C4%87%2C+D">D. Jokovi膰</a>, <a href="/search/physics?searchtype=author&query=Veselinovi%C4%87%2C+N">N. Veselinovi膰</a>, <a href="/search/physics?searchtype=author&query=Dragi%C4%87%2C+A">A. Dragi膰</a>, <a href="/search/physics?searchtype=author&query=Udovi%C4%8Di%C4%87%2C+V">V. Udovi膷i膰</a>, <a href="/search/physics?searchtype=author&query=Ani%C4%8Din%2C+I">I. Ani膷in</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1305.2572v2-abstract-short" style="display: inline;"> The background spectrum of a germanium detector, shielded from the radiations arriving from the lower and open for the radiations arriving from the upper hemisphere is studied, both in a ground level and in an underground laboratory. It is established that the continuous portion of this background spectrum is mostly due to the radiations that arrive from the upper hemisphere of the continuous spec… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1305.2572v2-abstract-full').style.display = 'inline'; document.getElementById('1305.2572v2-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1305.2572v2-abstract-full" style="display: none;"> The background spectrum of a germanium detector, shielded from the radiations arriving from the lower and open for the radiations arriving from the upper hemisphere is studied, both in a ground level and in an underground laboratory. It is established that the continuous portion of this background spectrum is mostly due to the radiations that arrive from the upper hemisphere of the continuous spectrum similar to the instrumental one. The intensity of this radiation of an average energy of about 120 keV is estimated to about 8000 photons/m2s 2蟺srad in a ground level laboratory, and to about 5000 photons/m2s 2蟺srad at the depth of 25 m.w.e. Rough estimates of the dose that it contributes to the skin are about 1.5 nSv/h and 1 nSv/h respectively. Simulations by GEANT4 and CORSIKA demonstrate that this radiation is both of cosmic and terrestrial origin, mixed in proportion that still has to be determined. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1305.2572v2-abstract-full').style.display = 'none'; document.getElementById('1305.2572v2-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 14 May, 2013; <span class="has-text-black-bis has-text-weight-semibold">v1</span> submitted 12 May, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> May 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">6 pages, 5 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1304.7879">arXiv:1304.7879</a> <span> [<a href="https://arxiv.org/pdf/1304.7879">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Atmospheric and Oceanic Physics">physics.ao-ph</span> </div> </div> <p class="title is-5 mathjax"> Further investigations into the connection between cosmic rays and climate </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Dragi%C4%87%2C+A">A. Dragi膰</a>, <a href="/search/physics?searchtype=author&query=Veselinovi%C4%87%2C+N">N. Veselinovi膰</a>, <a href="/search/physics?searchtype=author&query=Maleti%C4%87%2C+D">D. Maleti膰</a>, <a href="/search/physics?searchtype=author&query=Jokovi%C4%87%2C+D">D. Jokovi膰</a>, <a href="/search/physics?searchtype=author&query=Banjanac%2C+R">R Banjanac</a>, <a href="/search/physics?searchtype=author&query=Udovi%C4%8Di%C4%87%2C+V">V. Udovi膷i膰</a>, <a href="/search/physics?searchtype=author&query=Ani%C4%8Din%2C+I">I. Ani膷in</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1304.7879v1-abstract-short" style="display: inline;"> Our previous results on the connection between the Forbush decreases (FD) of cosmic-ray intensity and the deviations from the expected values of the diurnal temperature range (DTR) are briefly revisited. The same type of analysis is then extended to the cases of sudden increases of cosmic-ray intensity (GLE), as well as to the search for lattitude effects in the observed correlations. We find that… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1304.7879v1-abstract-full').style.display = 'inline'; document.getElementById('1304.7879v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1304.7879v1-abstract-full" style="display: none;"> Our previous results on the connection between the Forbush decreases (FD) of cosmic-ray intensity and the deviations from the expected values of the diurnal temperature range (DTR) are briefly revisited. The same type of analysis is then extended to the cases of sudden increases of cosmic-ray intensity (GLE), as well as to the search for lattitude effects in the observed correlations. We find that all the investigated correlations appear to manifest both the expected signs and the plausible phase relations, though each one only at the modest confidence level. Moreover, it appears that there is some proportionality between the magnitude of a cosmic-ray intensity change and a corresponding DTR deviation, both in the case of FD and GLE events. Eventual increase of the confidence levels at which these correlations are established would have to wait for the significant increase of the number of well defined and sufficiently intense recorded departures of cosmic-ray intensity from its stationary mean value. On the other hand, the probability of such an accidental multiple coincidence of independent pieces of evidence is certainly very low. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1304.7879v1-abstract-full').style.display = 'none'; document.getElementById('1304.7879v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 30 April, 2013; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> April 2013. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">9 pages, 3 figures</span> </p> </li> <li class="arxiv-result"> <div class="is-marginless"> <p class="list-title is-inline-block"><a href="https://arxiv.org/abs/1203.4607">arXiv:1203.4607</a> <span> [<a href="https://arxiv.org/pdf/1203.4607">pdf</a>] </span> </p> <div class="tags is-inline-block"> <span class="tag is-small is-link tooltip is-tooltip-top" data-tooltip="Instrumentation and Detectors">physics.ins-det</span> <span class="tag is-small is-grey tooltip is-tooltip-top" data-tooltip="Nuclear Experiment">nucl-ex</span> </div> <div class="is-inline-block" style="margin-left: 0.5rem"> <div class="tags has-addons"> <span class="tag is-dark is-size-7">doi</span> <span class="tag is-light is-size-7"><a class="" href="https://doi.org/10.2298/NTRP1101064N">10.2298/NTRP1101064N <i class="fa fa-external-link" aria-hidden="true"></i></a></span> </div> </div> </div> <p class="title is-5 mathjax"> The New Setup in the Belgrade Low-Level and Cosmic-Ray Laboratory </p> <p class="authors"> <span class="search-hit">Authors:</span> <a href="/search/physics?searchtype=author&query=Dragi%C4%87%2C+A">Aleksandar Dragi膰</a>, <a href="/search/physics?searchtype=author&query=Udovi%C4%8Di%C4%87%2C+V">Vladimir Udovi膷i膰</a>, <a href="/search/physics?searchtype=author&query=Banjanac%2C+R">Radomir Banjanac</a>, <a href="/search/physics?searchtype=author&query=Jokovi%C4%87%2C+D">Dejan Jokovi膰</a>, <a href="/search/physics?searchtype=author&query=Maleti%C4%87%2C+D">Dimitrije Maleti膰</a>, <a href="/search/physics?searchtype=author&query=Veselinovi%C4%87%2C+N">Nikola Veselinovi膰</a>, <a href="/search/physics?searchtype=author&query=Savi%C4%87%2C+M">Mihailo Savi膰</a>, <a href="/search/physics?searchtype=author&query=Puzovi%C4%87%2C+J">Jovan Puzovi膰</a>, <a href="/search/physics?searchtype=author&query=Ani%C4%8Din%2C+I+V">Ivan V. Ani膷in</a> </p> <p class="abstract mathjax"> <span class="has-text-black-bis has-text-weight-semibold">Abstract</span>: <span class="abstract-short has-text-grey-dark mathjax" id="1203.4607v1-abstract-short" style="display: inline;"> The Belgrade underground laboratory consists of two interconnected spaces, a ground level laboratory and a shallow underground one, at 25 m.w.e.. The laboratory hosts a low-background gamma spectroscopy system and cosmic-ray muon detectors. With recently adopted digital data acquisition system it is possible to study simultaneously independent operation of two detector systems, as well as processe… <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1203.4607v1-abstract-full').style.display = 'inline'; document.getElementById('1203.4607v1-abstract-short').style.display = 'none';">▽ More</a> </span> <span class="abstract-full has-text-grey-dark mathjax" id="1203.4607v1-abstract-full" style="display: none;"> The Belgrade underground laboratory consists of two interconnected spaces, a ground level laboratory and a shallow underground one, at 25 m.w.e.. The laboratory hosts a low-background gamma spectroscopy system and cosmic-ray muon detectors. With recently adopted digital data acquisition system it is possible to study simultaneously independent operation of two detector systems, as well as processes induced by cosmic-ray muons in germanium spectrometers. Characteristics and potentials of present experimental setup, together with some preliminary results for the flux of fast neutrons and stopped muons are reported. <a class="is-size-7" style="white-space: nowrap;" onclick="document.getElementById('1203.4607v1-abstract-full').style.display = 'none'; document.getElementById('1203.4607v1-abstract-short').style.display = 'inline';">△ Less</a> </span> </p> <p class="is-size-7"><span class="has-text-black-bis has-text-weight-semibold">Submitted</span> 20 March, 2012; <span class="has-text-black-bis has-text-weight-semibold">originally announced</span> March 2012. </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Comments:</span> <span class="has-text-grey-dark mathjax">12 pages, 16 figures</span> </p> <p class="comments is-size-7"> <span class="has-text-black-bis has-text-weight-semibold">Journal ref:</span> Nuclear Technology & Radiation Protection: Year 2011, Vol. 26, No. 3, pp.181-192 </p> </li> 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