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ASI Symposium 002

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font-size: 20px;font-weight:bold;" target="_blank">ASI SYMPOSIUM 002 POSTER</a>&nbsp;|&nbsp;&nbsp; </marquee> <section id="Register" class="py-5 bg-light"> <div class="container mt-5"> <!-- Registration Section --> <div class="row"> <!-- Registration Details Column --> <div class="col-md-6 mb-4"> <h2 class="mb-6">Event Registration</h2> <br> <p><strong>Registration Fee:</strong> Rs. 2000/-</p> <p>Please choose one of the registration options below:</p> <ul> <li>Invited Talk</li> <li>Contributed Talk: Oral/Poster</li> <li>Participant</li> </ul> <!-- Registration Link Section --> <a href="https://forms.gle/6YoiwMESoLfWBUzd9" target="_blank" class="btn btn-primary">Register Here</a> </div> <!-- Important Dates Column --> <div class="col-md-6"> <h3 class="mb-4">Important Dates</h3> <ul class="list-group"> <li class="list-group-item"> <strong>Registration and Abstract Submission Opens:</strong> <span class="highlight">01-10-2024</span> </li> <li class="list-group-item"> <strong>Abstract Submission Deadline (Oral and Poster):</strong> <span class="highlight">10.11.2024</span> </li> <li class="list-group-item"> <strong>Communication of Selected Oral and Poster Contributions:</strong> <span class="highlight">15.11.2024</span> </li> <li class="list-group-item"> <strong>Registration Deadline:</strong> <span class="highlight">02.12.2024</span> </li> <li class="list-group-item"> <strong>Last date for application for support:</strong> <span class="highlight">05.11.2024</span> </li> </ul> </div> </div> </div> </section> <!--<section id="Register" class="py-5 bg-light">--> <!-- <div class="container mt-5">--> <!-- Registration Section --> <!-- <h2 class="mb-4">Event Registration</h2>--> <!-- <p><strong>Registration Fee:</strong> Rs. 2000/-</p>--> <!-- <p>Please choose one of the registration options below:</p>--> <!-- <ul>--> <!-- <li>Invited Talk</li>--> <!-- <li>Contributed Talk: Oral/Poster</li>--> <!-- <li>Participant</li>--> <!-- </ul>--> <!-- Registration Link Section --> <!-- <a href="https://forms.gle/6YoiwMESoLfWBUzd9" target="_blank" class="btn btn-primary mb-4">Register Here</a>--> <!-- Important Dates Section --> <!-- <h3 class="mb-4">Important Dates</h3>--> <!-- <ul class="list-group">--> <!-- <li class="list-group-item">--> <!-- <strong>Registration and Abstract Submission Opens:</strong> <span class="highlight">[01-10-2024]</span>--> <!-- </li>--> <!-- <li class="list-group-item">--> <!-- <strong>Abstract Submission Deadline (Oral and Poster):</strong> <span class="highlight">[10.11.2024]</span>--> <!-- </li>--> <!-- <li class="list-group-item">--> <!-- <strong>Communication of Selected Oral and Poster Contributions:</strong> <span class="highlight">[15.11.2024]</span> --> <!-- </li>--> <!-- <li class="list-group-item">--> <!-- <strong>Registration Deadline:</strong> <span class="highlight">[02.12.2024]</span> --> <!-- </li>--> <!-- <li class="list-group-item">--> <!-- <strong>Last date for application for support: </strong> <span class="highlight">[05.11.2024]</span> --> <!-- </li>--> <!-- </ul>--> <!-- </div>--> <!-- </section>--> <div class="container"> <h2 class="text-center">Rationale</h2> <p class="text-justify mt-12" > The study of particle acceleration and transport is an important topic in Astrophysics, Heliophysics and Space-weather research. On the Sun and in the heliosphere, these particles are the sources of electromagnetic emissions at different wavelengths. Starting from electrons and protons to heavier ions are accelerated during the transient activities of the dynamic Sun. Energetic particle acceleration up to several MeV (electrons) and ions up to GeV have been studied theoretically and some of the results have been explored through experimental observations and modelling. Many of the spacecraft dedicated for solar and heliospheric observations have particle detectors of wide energy range. Also, solar energetic particle (SEP) events are one of the major causes of space weather impact on space-based technological systems. Impulsive SEP events are associated with solar flare reconnection sites while the gradual SEP events are accelerated by coronal mass ejection (CME) driven shocks . Many authors have proposed that the abundance of the ambient seed particles is also a determining factor in the large peak intensity of SEP events. These seed particles are believed to be supplied by flaring material from the preceding flares or coronal material from twin-CMEs. CME-driven shocks primarily accelerate protons and heavier ions, and differential elemental compositions and charge states are produced through different acceleration processes and seed populations. CME-driven shocks, in contrast to flares, have a much larger extent in the interplanetary medium. Gradual SEP events affect the natural and artificial satellites on their way. In addition, the abundance of particles in solar events, solar wind acceleration attracted the scientists recently. Large data base of particles from the sun is available from the space-based instruments like the recently launched spacecraft ADITYA L1. It has to be analysed and studied by solar data scientists. In general, a number of questions are to be discussed with experts in this field and presented to the younger audience (college/university research scholars, post-docs and teachers) from this part of geo-sphere. Hence the symposium on particle acceleration has been planned. </p> <p><h4>Theme: Particle Acceleration and Space Weather Impacts </h4> </p> <p>Astrophysical and Heliophysical Particle Acceleration</p> <p>Electromagnetic Emissions from Sun</p> <p>Solar Energetic Particles (SEPs) and Space Weather Effects</p> <p>Particle Detection in Space Missions (ADITYA L1, etc.)</p> <p>CME-Driven Shocks vs. Solar Flares: Acceleration Mechanisms</p> <p>Solar Wind and its effects</p> <p>Recent Advances in Theoretical and Experimental Observations</p> <p>Data Analysis and Modeling of Solar Events</p> </div> </section> <section id="Schedule" class="py-5 bg-light"> <div class="container mt-5"> <h2 class="text-center mb-4">ASI Symposium – Program Schedule</h2> <h4 class="text-center mb-4">16th - 18th December 2024</h4> <!-- Day 1 Table --> <h5 class="text-center text-primary">Day 1 – 16th December 2024 @ARUL ANANDAR COLLEGE</h5> <table class="table table-bordered table-striped table-hover"> <thead class="table-primary"> <tr> <th>Time</th> <th>Programme</th> <th>Name of the Resource Person</th> <th>Topic</th> </tr> </thead> <tbody> <tr> <td>9.150am-10:00 am</td> <td>Inauguration <br> Overview of the programme</td> <td>College management, SOC members <br> Dr.A.Shanmugaraju, Arul Anandar College</td> <td></td> </tr> <tr> <td>10.00am-10:30am</td> <td>Review Talk 1</td> <td>Dr.N.Gopalswamy, GSFC, NASA, USA</td> <td>Observational Signatures of Particle Energization on the Sun </td> </tr> <tr> <td>10.30am-10:50am</td> <td>Invited Talk 1</td> <td>Dr.Anshu Kumari, PRL, Ahmedabad.</td> <td>Theory of particle acceleration by shocks and radio bursts</td> </tr> <tr> <td>10.50am-11:30am</td> <td>Tea Break</td> <td></td> <td></td> </tr> <tr> <td>11.30am-1:00pm</td> <td>Contributed Talks</td> <td></td> <td></td> </tr> <tr> <td>1.00pm-2:00pm</td> <td>Lunch Break</td> <td></td> <td></td> </tr> <tr> <td>2.00pm-2:30pm</td> <td>Review Talk 2</td> <td>Dr.Bhuwan Joshi, USO,PRL,Udaipur</td> <td>Magnetic reconnection and Acceleration of particles revealed through multi-wavelength observations </td> </tr> <tr> <td>2.30pm-2:50pm</td> <td>Invited Talk 2</td> <td>Dr.M.Shanmugam, PIDS, PRL, Ahmedabad</td> <td>Particle detectors for space missions</td> </tr> <tr> <td>2.50pm-4.15pm</td> <td>Contributed Talks</td> <td></td> <td></td> </tr> <tr> <td>4.15pm-5.00pm</td> <td>Tea Break / Poster Session</td> <td></td> <td></td> </tr> <tr> <td>6.15pm-7.00pm</td> <td>Cultural Program</td> <td></td> <td></td> </tr> <tr> <td>7.00pm-8.00pm</td> <td>Symposium Banquet</td> <td></td> <td></td> </tr> </tbody> </table> <!-- Day 2 Table --> <h5 class="text-center text-primary">Day 2 – 17th December 2024 @ARUL ANANDAR COLLEGE</h5> <table class="table table-bordered table-striped table-hover"> <thead class="table-info"> <tr> <th>Time</th> <th>Programme</th> <th>Name of the Resource Person</th> <th>Topic</th> </tr> </thead> <tbody> <tr> <td>9.30am-9.45am</td> <td>Review of 1st day programme</td> <td>Dr.A.Shanmugaraju</td> <td></td> </tr> <tr> <td> 9.45am-10.15am</td> <td>Review Talk 3</td> <td>Dr.Rohith Sharma, IIT, Kanpur </td> <td>Particle acceleration using X-ray and radio observations</td> </tr> <tr> <td>10.15am-10.35am</td> <td>Invited Talk 3</td> <td>Dr.Ramesh Chandra, Kumaun University, Nainital</td> <td>Type II radio bursts and space weather phenomena</td> </tr> <tr> <td>10.35am-11.35am </td> <td>Tea Break & Poster Session</td> <td></td> <td></td> </tr> <tr> <td>11.35am-1.00pm</td> <td>Contributed Talks</td> <td></td> <td></td> </tr> <tr> <td>1.00pm-2.00pm</td> <td>Lunch Break</td> <td></td> <td></td> </tr> <tr> <td>2.00pm-2.30pm</td> <td>Review Talk 4</td> <td>Dr.Sasikumar Raja, IIA, Bangalore</td> <td>Properties of energetic electrons inferred from solar radio bursts </td> </tr> <tr> <td>2.30pm-2.50pm</td> <td>Invited Talk 4</td> <td>Dr.Arunbabu, Cochin University of Science & Tech, Kerala</td> <td>Forbush Decreases</td> </tr> <tr> <td>2.50pm-4.00pm </td> <td>Contributed Talks</td> <td></td> <td></td> </tr> <tr> <td> 4.00pm-4.45pm </td> <td> Tea break & Poster</td> <td></td> <td></td> </tr> <tr> <td> 5.00pm-5.30pm </td> <td> Closing session</td> <td>College management, SOC members</td> <td></td> </tr> </tbody> </table> <!-- Day 3 Table --> <h5 class="text-center text-primary">Day 3 – 18th December 2024</h5> <table class="table table-bordered table-striped table-hover"> <thead class="table-warning"> <tr> <th>Time</th> <th>Programme</th> </tr> </thead> <tbody> <tr> <td>All Day</td> <td>Kodaikanal Observatory Visit for interested participants (on extra payment)</td> </tr> </tbody> </table> </div> </section> <section id="Speakers" class="py-5 bg-light"> <div class="container mt-5"> <h2 class="text-center mb-4">ASI Symposium – List of Speakers</h2> <h3 class="text-center mb-4">As given in the schedule </h3> <!--<table class="table table-bordered table-striped table-hover"> <thead class="table-primary"> <tr> <th>Speaker</th> <th>Affiliation</th> <th>Topic</th> </tr> </thead> <tbody> <tr> <td>Dr. N. Gopalswamy</td> <td>NASA, USA</td> <td>Review talk on SEPs and Space weather</td> </tr> <tr> <td>Dr. R. Ramesh</td> <td>IIA</td> <td>Review talk on Observation of Solar Radio bursts</td> </tr> <tr> <td>Dr. Janardhan Padmanaban</td> <td>PRL</td> <td>Review talk on Solar wind particles</td> </tr> <tr> <td>Dr. Wageesh Misra</td> <td>IIA, Bangalore</td> <td>Interacting CMEs and SEPs</td> </tr> <tr> <td>Dr. Ramesh Chandra</td> <td>Kumaun University, Nainital</td> <td>Small SEP Events</td> </tr> <tr> <td>Dr. B. Veenadhari</td> <td>IIGM</td> <td>SEP interaction with atmosphere – Aurora</td> </tr> <tr> <td>Dr. Selvakumaran</td> <td>AMITY University</td> <td>Type II radio bursts and IP shocks</td> </tr> <tr> <td>Dr. Srikar Paavan Tadepalli</td> <td>URSC</td> <td>Particle acceleration from Aditya-L1</td> </tr> <tr> <td>Dr. Nandita Srivastava</td> <td>PRL</td> <td>SEPs and Geomagnetic storms (Energetic Storm Particle Events)</td> </tr> <tr> <td>Dr. Bhuwan Joshi</td> <td>PRL</td> <td>Solar eruptions and acceleration of particles</td> </tr> <tr> <td>Dr. Anshu Kumari</td> <td>PRL</td> <td>Radio bursts in Solar cycle 23 and 24</td> </tr> <tr> <td>Dr. M. Shanmugam</td> <td>PRL</td> <td>Particle detectors for space missions</td> </tr> <tr> <td>Dr. Dibeyandu Chakrabarthi</td> <td>PRL</td> <td>Aurora</td> </tr> <tr> <td>Dr. Divya Oberoi</td> <td>NCRA</td> <td>Electron acceleration from the Sun</td> </tr> <tr> <td>Dr. Sasikumar Raja</td> <td>IIA</td> <td>Ground and space based observations of solar radio type III bursts</td> </tr> <tr> <td>Dr. Vema Reddy</td> <td>IIA</td> <td>Space weather events</td> </tr> <tr> <td>Raj K. Choudhariy</td> <td>VSSC, Trivandrum</td> <td>SEP influence on the ionosphere</td> </tr> <tr> <td>Dr. Firoza K. Sutaria</td> <td>IIA</td> <td>Shock acceleration in supernova</td> </tr> <tr> <td>Dr. Arun Babu</td> <td>CUSAT, Kerala</td> <td>Forbush decreases</td> </tr> <tr> <td>Dr. Hariharan Balakrishnan</td> <td>CRL-TIFR, Ooty</td> <td>Muon Anisotropy</td> </tr> <tr> <td>Dr. Sunder Sahayanathan</td> <td>BARC</td> <td>Acceleration process in the jets of AGN</td> </tr> <tr> <td>Dr. Stalin</td> <td>IIA</td> <td>AGN (Active Galactic Nuclei) and the shocks associated</td> </tr> <tr> <td>Dr. Prateek Sharma</td> <td>IISc</td> <td>Extra-galactic shocks</td> </tr> <tr> <td>Dr. Bhargav Vaidya</td> <td>IIT Indore</td> <td>Shocks</td> </tr> <tr> <td>Dr. Ranjiv Mishra</td> <td>IUCCA</td> <td>X-ray binary and shocks</td> </tr> <tr> <td>Dr. Dipankar Bhattacharya</td> <td>Ashoka University</td> <td>High energy astrophysics</td> </tr> </tbody> </table>--> </div> </section> <section id="Abs" class="py-5 bg-light"> <div class="container"> <h2 class="text-center">Abstract</h2> <p class="text-justify mt-12" > <p><b>Abstract submission:</b></p> <p>Submit the abstract through the registration form ( <a href="https://forms.gle/6YoiwMESoLfWBUzd9" class="text-black">Reg link: https://forms.gle/6YoiwMESoLfWBUzd9 )</a> </p> <p><b>Abstract Format:</b></p> <p>Abstract title followed by authors and their address, email </p> <p><b>Font:</b> Times New Roman, Font size - 12, Single line spacing, </p> <p>Should be submitted in MsWord Format</p> <p><b>Eligibility to submit the abstract:</b></p> <p>Researchers across India are invited to submit abstracts in the prescribed format related to the theme of the symposium. Apart from 6-8 invited talks, a set of contributed talks will be selected from the submitted abstracts related to the theme of the symposium. The remaining accepted abstracts will be presented as poster papers</p> </p> <p><b>Support</b></p> <p>Support for Ph.D. students: A limited fund is available for research scholars for their registration/travel/accommodation. Based on the decision of SOC, this support may be provided based on the request from the scholars via email to the convenor(<a href="shanmugaraju@aactni.edu.in" class="text-black">shanmugaraju@aactni.edu.in</a> ). </p> <p>Who can attend: College/University/Research Organization research scholars, post-docs and teachers in India</p> <p><b>Last date for application for support: 05.11.2024</b></p> </p> <center><p><h3><b>Oral Presentation</b></h3></p></center> <table class="table table-bordered table-striped table-hover"> <thead> <tr> <th>#</th> <th>Name</th> <th>Title</th> <th>Institution</th> </tr> </thead> <tbody> <tr> <td>1</td> <td>K. Sankarasubramanian</td> <td>Particle Acceleration Studies with Aditya-L1</td> <td>URSC, ISRO, Bangalore</td> </tr> <tr> <td>2</td> <td>K. P. Arunbabu</td> <td>Signatures of Particle Acceleration within the Interplanetary Magnetic Flux Ropes</td> <td>Cochin University of Science and Technology</td> </tr> <tr> <td>3</td> <td>Mahender Aroori</td> <td>Statistical Study of Spatial and Temporal Characteristics of Solar Flares during Solar Cycle 24</td> <td>Osmania University</td> </tr> <tr> <td>4</td> <td>Sruthi Mildred</td> <td>Impact of two consecutive interplanetary shocks on plasma waves and particle dynamics in Earth’s magnetosphere</td> <td>Cochin University of Science and Technology</td> </tr> <tr> <td>5</td> <td>P. Vijayalakshmi</td> <td>Association of an intense geomagnetic storm driven by a Radio-Loud coronal mass ejection (CME) and solar energetic particles (SEPs) with solar source</td> <td>Arul Anandar College</td> </tr> <tr> <td>6</td> <td>K. Suresh</td> <td>Studying Earth-Directed CME Deflection through Coronal Dimmings and Coronal Holes Analysis</td> <td>PSR Engineering College, Sivakasi</td> </tr> <tr> <td>7</td> <td>K. Mahalakshmi</td> <td>Study of solar proton events in the rising phase of the solar cycle 25</td> <td>United Institute of Technology, Coimbatore</td> </tr> <tr> <td>8</td> <td>Debi Prasad Choudhary</td> <td>Thermal, Magnetic and Velocity Properties in Source Region of Solar Activity</td> <td>California State University Northridge</td> </tr> <tr> <td>9</td> <td>S. Prasanna Subramanian</td> <td>Study of Earthquakes and their relation with solar activities</td> <td>HKRH College, Uthamapalayam</td> </tr> <tr> <td>10</td> <td>Ritesh Sharma</td> <td>A framework for modelling CME propagation</td> <td>University of South Bihar</td> </tr> <tr> <td>11</td> <td>Pooja Devi</td> <td>Prominence Eruption and Associated Loop Contraction</td> <td>Kumaun University, Nainital</td> </tr> <tr> <td>12</td> <td>A. Kubera Raja</td> <td>Major solar energetic particles and their relationship to associated flares and CMEs</td> <td>Government College of Engineering, Bodinayakkanur</td> </tr> <tr> <td>13</td> <td>Shaik Sayuf</td> <td>Estimation of Solar coronal magnetic field strength at meter wavelengths using augmented Gauribidanur RadioheliograPH (GRAPH)</td> <td>Indian Institute of Astrophysics, Bangalore</td> </tr> <tr> <td>14</td> <td>Bendict Lawrance</td> <td>Comparative Analysis of ICME Characteristics and Geoeffectiveness across Solar Cycles 23, 24 and 25</td> <td>Gangseo University, Republic of Korea</td> </tr> <tr> <td>15</td> <td>Suganya Sundaramurthy</td> <td>Estimating the coronal magnetic field strength via CME-driven shocks: A comprehensive evaluation of stand-off distance (SOD) method</td> <td>Indian Institute of Astrophysics, Bangalore</td> </tr> <tr> <td>16</td> <td>Annalakshmi Muppudathi</td> <td>Effect of Coronal Mass Ejections during Lunar Phases of Full moon day and New moon day</td> <td>Periyar University, Salem</td> </tr> <tr> <td>17</td> <td>S. Aswin Amirtha Raj</td> <td>Trustworthiness of Sunspot’s Magnetic Parameters in Predicting Coronal Mass Ejection Velocity</td> <td>Arul Anandar College, Madurai</td> </tr> <tr> <td>18</td> <td>Sushree Sangeeta Nayak</td> <td>Studying flare ribbon dynamics using MHD simulation</td> <td>Center for Space Plasma and Aeronomic Research, the University of Alabama, USA</td> </tr> <tr> <td>19</td> <td>M. Syed Ibrahim</td> <td>Geo-effectiveness of non-active region interplanetary CMEs: initiation, propagation and near-Earth consequences</td> <td>Sri Sai Ram Engineering College, Chennai</td> </tr> <tr> <td>20</td> <td>G. Selvarani</td> <td>Observations of radio bursts association with halo CMEs and M-class solar flares</td> <td>Sri Meenakshi Government Arts College for Women, Madurai</td> </tr> <tr> <td>21</td> <td>P. Pappa Kalaivani</td> <td>Study on quick and delayed major SEPs based on the onset of type II radio bursts</td> <td>Ultra College of Engineering & Technology, Madurai</td> </tr> <tr> <td>22</td> <td>A. Mujiber Rahman</td> <td>Radio analysis of solar activities associated with 25 Feb 2014 day event</td> <td>HKRH College, Uthamapalayam</td> </tr> <tr> <td>23</td> <td>W. Hannah Blessy</td> <td>Investigations on coronal mass ejections associated with flares and DH type II radio bursts of solar cycle 25 from January 2020 to December 2023</td> <td>The American College, Madurai.</td> </tr> </tbody> </table> <center><p><h3><b>Poster Presentation</b></h3></p></center> <table class="table table-bordered table-striped table-hover"> <thead> <tr> <th>#</th> <th>Name</th> <th>Title</th> <th>Institution</th> </tr> </thead> <tbody> <tr> <td>1</td> <td>K. Suresh</td> <td>Examining CME-Driven Type II Radio Bursts: Insights from Multi-Instrument Observations from Solar Cycle 24</td> <td>PSR Engineering College, Sivakasi</td> </tr> <tr> <td>2</td> <td>A. Ansar Ahamed</td> <td>Study of a Halo CME and its Associated Activities observed on March 23, 2024</td> <td>Hajee Karutha RowtherHowdia College, Uthamapalayam</td> </tr> <tr> <td>3</td> <td>M. Syed Ibrahim</td> <td>Transit time of CME/shock associated with a major geo-effective CME in solar cycle 25</td> <td>Sri Sai Ram Engineering College, Chennai</td> </tr> <tr> <td>4</td> <td>A. Alexander</td> <td>Solar wind and climate change on the Earth</td> <td>St. Joseph’s College (Autonomous) Tiruchirappalli</td> </tr> <tr> <td>5</td> <td>Sunil Yadav</td> <td>Discerning the contribution of small and large-scale magnetic fields on the X-ray flux of the Sun</td> <td>IISER Berhampur</td> </tr> <tr> <td>6</td> <td>RJ Anjana Shree</td> <td>Temperature profile of Martian lower atmosphere and study its variation with seasons, through the day and with solar activity</td> <td>Thiagarajar College, Madurai</td> </tr> <tr> <td>7</td> <td>R. Sindhan</td> <td>On the Effective Rotational Temperature of Large Sunspot Umbra using System of CaH Molecule</td> <td>N.M.S.S.V.N. College, Madurai</td> </tr> <tr> <td>8</td> <td>K. Subbu Ulaganatha Pandian</td> <td>Investigation on Coronal Mass Ejections and Groups of Type III Radio Bursts during Solar Cycle 23</td> <td>Bharathiar University, Coimbatore</td> </tr> <tr> <td>9</td> <td>N. Yogeswaran</td> <td>Investigations of changes in sunspot properties leading to coronal mass ejections</td> <td>Arul Anandar College, Madurai</td> </tr> <tr> <td>10</td> <td>Kere Ravi Arjun</td> <td>Mars Perseverance Images to Validate Solar Far-Side Active Regions</td> <td>IISER Mohali</td> </tr> <tr> <td>11</td> <td>P. Jawahar Raja</td> <td>Determining filament counts using H-alpha images of the Sun</td> <td>Dr. N.G.P Arts and Science College, Coimbatore</td> </tr> <tr> <td>12</td> <td>J. Poojapriyatharsheni</td> <td>Survey of H, He, and C radio recombination lines in the inner Galactic plane and the Cygnus-X region</td> <td>Lady Doak College, Madurai</td> </tr> <tr> <td>13</td> <td>A. Raj Krishnan</td> <td>Investigations on coronal mass ejections of solar cycle 25 from January 2020 to December 2023</td> <td>The American College, Madurai</td> </tr> <tr> <td>14</td> <td>M. Manivasuki</td> <td>Relationship between CME activity, geomagnetic storms, and precipitation pattern during rainy seasons</td> <td>Periyar University, Salem</td> </tr> <tr> <td>15</td> <td>C. Revathi</td> <td>Forecasting seasonal climate trends during coronal mass ejections activity</td> <td>Periyar University, Salem</td> </tr> <tr> <td>16</td> <td>P.P. Kannan</td> <td>On the Effective Rotational Temperature of Large Sunspot Umbra using C2 Molecule</td> <td>M.T.N. College, Madurai</td> </tr> <tr> <td>17</td> <td>N. Venkatesh Bharathi</td> <td>Computation of Radiative Transition Parameters of Dicarbon (C2) molecule in the high temperature atmosphere, S-stars and sunspots</td> <td>M.T.N. College, Madurai</td> </tr> <tr> <td>18</td> <td>Divya Kumari</td> <td>Unraveling Solar Explosions: Insights into CME and ICME Dynamics through Multi-Wavelength Observations</td> <td>Jai Prakash University, Chapra, Bihar</td> </tr> </tbody> </table> </div> </section> <section id="Travel" class="py-5 bg-light"> <div class="container"> <!-- Contact Information --> <div class="row"> <div class="col-md-6 mb-4"> <h4>Travel and Accommodation </h4> <p>Arul Anandar College is located nearly 20 km away from Madurai city <a href="https://maps.app.goo.gl/ndm8eAkn9zwApiRB6" class="text-black">https://maps.app.goo.gl/ndm8eAkn9zwApiRB6</a> </p><p>To facilitate easy transport, we arranged a pickup vehicle from Kalavasal (~1km from Madurai Railway station) </p> <p>The Hostel facilities are limited. It can accommodate around 20 Research scholars at a cost of Rs.500 per day. Scholars can send a request through email to convenor for free accommodation.</p> <p><h3>Hotel List</h3></p> <p><b>Near Madurai Railway station (~ 22km to college)</b></p> <p>Mani&#39;s residency</p> <p>Hotel YMCA - Near Meenakshi Amman Temple Madurai</p> <p>The Grand Sabarees</p> <p>Hotel New College House</p> <p>Cosmopolitan Hotels</p> <p>Hotel Supreme</p> <p>Weshtern Park hotel</p> <p><b>Near Madurai Kalavasal (~ 20km to college)</b></p> <p>Hotel Germanus</p> <p>Hotel Jeyasakthi</p> <p>Hotel Ramtel Inn</p> </div> </div> </div> </section> <section id="foo" class="py-5 bg-light"> <footer class="bg-dark text-white mt-5 pt-4"> <div class="container"> <!-- Contact Information --> <div class="row"> <div class="col-md-6 mb-4"> <h5>Organizing Committee Under the Partonage of </h5> <p> Rev. Dr. John Pragasam S.J.</p> <p>Rector, Arul Anandar College</p> <p> Rev. Dr. Antonysamy A S.J.</p> <p>Secretary, Arul Anandar College</p> <p> Rev. Dr. Anbarasu M S.J. </p> <p> Principal, Arul Anandar College</p> <h5>Contact</h5> <p><strong>Chair:</strong> Dr. A. Shanmugaraju</p> <p>Associate Prof. and Head, PG and Research Dept. of Physics,<br> Arul Anandar College, Karumathur-625 514,<br> Madurai Dist., Tamilnadu</p> <p>Email: <a href="ashanmugaraju@gmail.com" class="text-white">ashanmugaraju@gmail.com</a></p> <p>Phone: 9842982672</p> <p><strong>Scholars:</strong></p> <ul> <li>Mr. Aswin Amirtharaj (7200033499)</li> <li>Ms. P. Vijayalakshmi (9283763626)</li> </ul> </div> <!-- LOC Information --> <div class="col-md-6 mb-4"> <h5>Local Organizing Committee (LOC)</h5> <ul> <li>Dr. K. S. Joseph Wilson, Associate Professor, Arul Anandar College</li> <li>Dr. A. Shanmugaraju, Associate Prof. & Head (Chair), Arul Anandar College</li> <li>Dr. S. Valanarasu, Assistant Professor, Arul Anandar College</li> <li>Dr. J. Sophia, Assistant Professor, Arul Anandar College</li> <li>Dr. C. S. A. Raj, Assistant Professor, Arul Anandar College</li> <li>Dr. S. Sebastian, Assistant Professor, Arul Anandar College</li> <li>Dr. M. Antony, Assistant Professor, Arul Anandar College</li> <li>Dr. I. Inigo Valan, Assistant Professor, Arul Anandar College</li> <li>Dr. P. Diana, Assistant Professor, Arul Anandar College</li> </ul> </div> </div> <!-- SOC Information --> <div class="row"> <div class="col-md-6 mb-4"> <h5>Scientific Organizing Committee (SOC)</h5> <ul> <li>Dr. A. Shanmugaraju, Arul Anandar College, Madurai</li> <li>Dr. C. Kathiravan, Indian Institute of Astrophysics, Bangalore</li> <li>Dr. S. P. Rajaguru, Indian Institute of Astrophysics, Bangalore</li> <li>Dr. Piyali Chatterjee, Indian Institute of Astrophysics, Bangalore</li> <li>Dr. Durgesh Tripathi, IUCAA, Pune</li> <li>Dr. A. K. Srivastava, IIT BHU, Varanasi</li> <li>Dr. K. Sankarasubramanian, ISRO, Bangalore</li> <li>Dr. Nitin Yadav, IISER, Thiruvananthapuram, Kerala</li> <li>Dr. G. Selvarani, Sri Meenakshi Govt College for Women, Madurai</li> </ul> </div> <!-- Location Information --> <div class="col-md-6 mb-4"> <h5>Location</h5> <p>Arul Anandar College (Autonomous), Karumathur, Madurai, Tamil Nadu</p> <p><a href="#" class="text-white">View on Map</a></p> <h5>Hotels Nearby</h5> <p>Details of nearby hotels can be found <a href="#" class="text-white">here</a>.</p> </div> </div> <!-- About the College and Department --> <div class="row"> <div class="col-md-12"> <h5>About the Institution</h5> <p>Arul Anandar College (Autonomous) is a Jesuit Minority Catholic Institution, affiliated with Madurai Kamaraj University, located 20km from Madurai City. Established in 1970, it was granted autonomous status in 1987 by UGC and the Government of Tamil Nadu. The college is accredited with an 'A' grade by NAAC (Cycle IV) and focuses on molding students into responsible citizens through education.</p> <h5>About the Department of Physics</h5> <p>Established in 1971, the Department of Physics offers B.Sc. and M.Sc. degrees under the Choice Based Credit System (CBCS) and Outcome Based Education (OBE). The department has been a recognized research center of Madurai Kamaraj University since 2013. Faculty members specialize in fields like Photonics, Astrophysics, Thin Films, and Nanoscience, and are engaged in UGC, DST, TNSCST, and DAE projects, guiding Ph.D. scholars on both part-time and full-time bases.</p> </div> </div> </div> <!-- Footer Bottom --> <div class="bg-secondary text-center py-3"> <p class="mb-0">&copy; 2024 Arul Anandar College. All Rights Reserved.</p> </div> </footer> </section> <!-- Bootstrap JS and dependencies --> <script src="https://cdn.jsdelivr.net/npm/bootstrap@5.3.0-alpha1/dist/js/bootstrap.bundle.min.js"></script> </body> </html>

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