Collisionless resistivity and velocity power spectrum for the geomagnetic tail-Reference-Cited by-同舟云学术

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Collisionless resistivity and velocity power spectrum for the geomagnetic tail

Published:1995 Issue: Volume: Page:223-231
ISSN:0065-8448
Container-title:Space Plasmas: Coupling Between Small and Medium Scale Processes
language:
Short-container-title:

Author:

Horton W.,Hernandez J.,Tajima T.

Publisher

American Geophysical Union

Reference36 articles.

1. Need for a three-dimensional analysis of magnetic fields in the magnetotail during substorms;Akasofu;Geophys. Res. Lett.,1978

2. The solar wind-magnetosphere energy coupling and magnetospheric disturbances;Akasofu;Planet. Space Sci.,1980

3. Energy coupling between the solar wind and the magnetosphere;Akasofu;Space Sci. Rev.,1981

4. A particle simulation of the tearing mode instability at the day side magnetopause;Allen;J. Geophys. Res.,1989

5. The evolution from weak to strong geomagnetic activity: An interpretation in terms of deterministic chaos;Baker;Geophys. Res. Lett.,1990

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