Solar wind-magneto sphere coupling: A review of recent results

Research output: Contribution to journalArticleScientificpeer-review

Researchers

Research units

  • Los Alamos Natl Lab, Los Alamos National Laboratory, United States Department of Energy (DOE)
  • St. Petersburg State University
  • Finnish Meteorological Institute

Abstract

This paper reviews some aspects of solar wind-magnetosphere-ionosphere interaction. It is shown that in addition to the interplanetary electric field, the solar wind dynamic pressure also has a significant role in determining the state, dynamics, and energetics of the system. It is demonstrated how the state of the magnetosphere and the prior driving affect the amount of energy input to the system, which highlights the capability of the magnetosphere to control the energy flow. The active role of the magnetosphere in determining the dynamics is illustrated by statistical results of the flux balance in the magnetotail and the various dynamic cycles the system can enter. The inner magnetosphere processes during storms are shown to be a result of a complex interplay of processes at the magnetopause and in the magnetotail in response to the solar wind driving. The conclusions are drawn from statistical observational results, empirical models, and global MHD simulations. (c) 2006 Published by Elsevier Ltd.

Details

Original languageEnglish
Pages (from-to)256-264
Number of pages9
JournalJOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS
Volume69
Issue number3
Publication statusPublished - Mar 2007
MoE publication typeA1 Journal article-refereed
EventYosemite Workshop on Global Aspects of Magnetosphere-Ionosphere Coupling - Yosemite, Canada
Duration: 7 Feb 200610 Feb 2006

    Research areas

  • substorms, storms, energy budget, magnetotail, PRESSURE, STORMS, SHEET, DST

ID: 2605333