Task 3

From CAWSES

Revision as of 05:34, 4 January 2010 by Pfox (Talk | contribs)
Jump to: navigation, search

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

Organizational Structure

Project 1. CME-ICME connection (Kinematics magnetic flux and helicity, charge state)

  • Project Chair: K. Kusano
  • Project members: TBD

Project 2.Shock formation in the solar atmosphere (CME, radio bursts, SEP , EIT waves)

  • Project Chair: Y. Yan
  • Project members: TBD

Project 3. Coronal hole and high speed solar Wind (comparisonwith ICME and CIR)

  • Project Chair: M. Shimojo
  • Project members: TBD

Project 4 Solar wind-Magnetosphere interface (Energy transfer from the solar wind to the magnetosphere)

  • Project Chair: T. Ogino
  • Project members: TBD

Project 5. 3 D structures of ICME and of Solar Wind

  • Project Chair: B. Jackson
  • Project members: TBD

Project 6. Substormvariability

  • Project Chair: B.T. Tsurutani
  • Project members: TBD

Project 7. Origin and emergence of solar magnetism

  • Project Chair: S. Brun
  • Project members: TBD

Introduction

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