Difference between revisions of "Working Group 3"
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===''Initiation''=== | ===''Initiation''=== | ||
| − | ===''Propagation''=== | + | ==='''Propagation'''=== |
| − | ===''Impact''=== | + | ===''''Impact''''=== |
==Simulation of Event Periods (with WG1)== | ==Simulation of Event Periods (with WG1)== | ||
Revision as of 23:22, 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'
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
