Difference between revisions of "ISEST 2015 Workshop"

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(WG2 Theory Group Presentation (October 27, 2015, Tuesday))
(WG1 Data Group Presentations (October 26, 2015, Monday))
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==WG1 Data Group Presentations (October 26, 2015, Monday)==
 
==WG1 Data Group Presentations (October 26, 2015, Monday)==
*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/WG1_data/Bothmer_Forecasting_Magnetic_Field_Configuration.pdf the Magnetic Field Configuration of CMEs --- by Volker Bother* (Invited)] <br>
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*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/WG1_data/Bothmer_Forecasting_Magnetic_Field_Configuration.pdf Forecasting the Magnetic Field Configuration of CMEs --- by Volker Bother* (Invited)] <br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/WG1_data/Yermolaev_Average_Behavior_Disturbed_SW.pdf  Average Behavior of Disturbed Type of Solar Wind --- by Yuri Yermolaev*, I. G. Lodkina, N. S.  Nikolaeva, M. Yu. Yermolaev] <br>
 
*[http://solar.gmu.edu/wiki/presentations/ISEST_2015_workshop/WG1_data/Yermolaev_Average_Behavior_Disturbed_SW.pdf  Average Behavior of Disturbed Type of Solar Wind --- by Yuri Yermolaev*, I. G. Lodkina, N. S.  Nikolaeva, M. Yu. Yermolaev] <br>
 
*Predicting ICME Signatures at L1 With a  Data-Constrained Physical Model --- by Phillip Hess*, J. Zhang <br>
 
*Predicting ICME Signatures at L1 With a  Data-Constrained Physical Model --- by Phillip Hess*, J. Zhang <br>

Revision as of 12:49, 28 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)

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