Difference between revisions of "Working Group 3"
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* Impact | * Impact | ||
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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? | ||
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* The CME-associated phenomena | * The CME-associated phenomena | ||
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* Arrival time | * Arrival time | ||
* Geo-effectiveness | * Geo-effectiveness | ||
Revision as of 23:57, 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 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
