Difference between revisions of "Working Group 3"
(→Simulations, Data, Results) |
(→Scientific Objective) |
||
| Line 2: | Line 2: | ||
==Scientific Objective== | ==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== | ==Scientific Questions== | ||
Revision as of 22:06, 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
Simulations, Data, Results
