Difference between revisions of "ISEST 2015 Workshop"

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(WG3 Simulation Group Presentations (October 27, 2015, Tuesday))
(WG Report (October 26, 2015, Monday))
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/working_group_report/WG1_report_Zhang.pdf WG1 data Group Report ---- by Jie Zhang] <br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/working_group_report/WG1_report_Zhang.pdf WG1 data Group Report ---- by Jie Zhang] <br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/working_group_report/WG2_report_Riley_Vrsnak.pdf WG2 Theory Group Report ---- by Peter Riley*, Bojan Vrsnak] <br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/working_group_report/WG2_report_Riley_Vrsnak.pdf WG2 Theory Group Report ---- by Peter Riley*, Bojan Vrsnak] <br>
*WG3 Simulation Group Report ---- by Noe Lugaz*, Fang Shen <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/working_group_report/WG3_report_Lugaz_Shen.pdf Simulation Group Report ---- by Noe Lugaz*, Fang Shen] <br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/working_group_report/WG4_report_Webb.pdf WG4 Campaign Study Group Report ---- by David Webb]<br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/working_group_report/WG4_report_Webb.pdf WG4 Campaign Study Group Report ---- by David Webb]<br>
 
*WG5 Bs Challenge Group Report ---- by Volker Bothmer*, Spiros Patsourakos <br>
 
*WG5 Bs Challenge Group Report ---- by Volker Bothmer*, Spiros Patsourakos <br>

Revision as of 17:55, 27 October 2015

This page contains presentations given at the 2015 ISEST Workshop. The 2015 ISEST Workshop was held in October 26-30, 2015, Mexico City, Mexico. Here is the link to the meeting website

WG Report (October 26, 2015, Monday)

WG1 Data Group Presentations (October 26, 2015, Monday)

WG2 Theory Group Presentation (October 27, 2015, Tuesday)

  • Coronal Mass Ejections: A Journey From Its Origin to Its Transport in the Interplanetary Medium --- by Andrea Borgazzi* (Invited Talk)
  • Balance of Energy in a CME --- by Héctor J. Durand Manterola*
  • Plasma Interaction Processes That Lead to Viscous Forces in the Solar Wind --- by Héctor Pérez de Tejada*
  • Synthetic Transits of Plasma Sheaths and Shocks: A Pathway to Predict in-situ Arrivals of Shock Waves Associated With Fast Halo CMEs --- by Pedro Corona Romero*, J. A. González Esparza, V. de la Luz, J. C. Mejía Ambriz, L. X. González
  • Dynamics of Coronal Mass Ejections in the Interplanetary Medium in Two Dimensions --- by Juan Carlos González Marin*
  • Study of the Transport of Heat in the Solar Corona --- by Diana Gamborino Uzcanga*, J. Martinell Benito, D. del Castillo Negrete

WG3 Simulation Group Presentations (October 27, 2015, Tuesday)

  • MHD Simulation of Interplanetary Propagation of Multiple Coronal Mass Ejections With Internal Magnetic Flux Rope --- by Daikou Shiota* (Invited Talk)
  • Parametric Functions of Coronal Mass Ejections Properties Close to the Sun Based on Numerical Hydrodynamic Simulations --- by R. González Domínguez, Tatiana Niembro Hernández*, A. Lara, J. Cantó
  • Simulation of Ground Level Enhancements and Forbush Decreases Using High Altitude Water Cherenkov Observatory (HAWC) Scalar System --- by Olivia Enríquez* Rivera, A. Lara, R. Caballero López
  • Shock Propagating Inside CMEs: Properties and Impact on Geospace --- by Noé Lugaz*
  • Review on Super-elastic Collision Between Plasmoids --- by Julio Herrera*, T. Niembro, A. Lara
  • Understanding the nature of collisions of CMEs in the hemisphere --- by Wageesh Mishra*, Nandita Srivastava
  • Turn on the Super-elastic Collision Nature of Coronal Mass Ejections Through Low Approaching Speed --- by Fang Shen, Yuming Wang*, Chenglong Shen, XueShang Feng