Task 3

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=How does short-term solar variability affect the geospace environment?=
=How does short-term solar variability affect the geospace environment?=
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==Introduction==
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==Organizational Structure==
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==Scientific Issues==
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'''[[Task 3 Project 1|Project 1. CME-ICME connection (Kinematics magnetic flux and helicity, charge state)]]'''
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The scientific issues of the Task Group 3 are as follows.
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* Project Chair: K. Kusano
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* Project members: TBD
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'''[[Task 3 Project 2|Project 2.Shock formation in the solar atmosphere (CME, radio bursts, SEP , EIT waves)]]'''
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=== ===
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* Project Chair: Y. Yan
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* Project members: TBD
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'''[[Task 3 Project 3|Project 3. Coronal hole and high speed solar Wind (comparisonwith ICME and CIR)]]'''
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* Project Chair: M. Shimojo
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* Project members: TBD
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'''[[Task 3 Project 4.|Project 4 Solar wind-Magnetosphere interface (Energy transfer from the solar wind to the magnetosphere)]]'''
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* Project Chair: T. Ogino
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* Project members: TBD
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'''[[Task 3 Project 5|Project 5. 3 D structures of ICME and of Solar Wind]]'''
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* Project Chair: B. Jackson
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* Project members: TBD
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'''[[Task 3 Project 6|Project 6. Substormvariability]]'''
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* Project Chair: B.T. Tsurutani
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* Project members: TBD
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'''[[Task 3 Project 7|Project 7. Origin and emergence of solar magnetism]]'''
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* Project Chair: S. Brun
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* Project members: TBD
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==Introduction==
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Revision as of 05:18, 26 November 2010

Contents

How does short-term solar variability affect the geospace environment?

Introduction

Scientific Issues

The scientific issues of the Task Group 3 are as follows.

Retrieved from "http://cawses.org/wiki/index.php/Task_3"
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