Difference between revisions of "Working Group 3"
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==Results of Numerical Simulations== | ==Results of Numerical Simulations== | ||
| − | == | + | ==Simulation of Event Periods (with WG1)== |
* late July to early August 2010 | * late July to early August 2010 | ||
Revision as of 23:19, 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)
Contents
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
Investigation of 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
