Difference between revisions of "Working Group 3"

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(Results of Numerical Simulations)
(Mechanisms, processes, and forces (with WG2))
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* July 2012
 
* July 2012
  
===''Mechanisms, processes, and forces (with WG2)''===
+
==Mechanisms, processes, and forces (with WG2)==
  
 
* How much variable ambient conditions affect ICMEs?
 
* How much variable ambient conditions affect ICMEs?

Revision as of 23:18, 6 June 2013

Simulation group led by Dusan Odstrcil (USA) and Fang Shen (China); At-large leaders: Noe Lugaz (USA) and Chin-Chun Wu (USA)

Scientific Objective

  • Provide global context for all CME events investigated by the ISEST team
  • Investigate processes of the CME initiation and heliospheric propagation
  • Develop tools to assist collaboration of numerical modelers, theoreticians, and observers

Scientific Questions

Initiation

Propagation

Impact

Results of Numerical Simulations

Simulation of Event Periods (with WG1)

  • late July to early August 2010
  • February 2011
  • early March 2012
  • July 2012

Mechanisms, processes, and forces (with WG2)

  • How much variable ambient conditions affect ICMEs?
  • Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?
  • The CME-associated phenomena

Forecasting the CME arrival and impacy (with WG4)

  • Arrival time
  • Geo-effectiveness
  • Energetic particles

Future Plan

TBD