Geomagnetic tail oscillations in quasihydrodynamics

A. I. Ershkovich, S. A. Martjanov

Research output: Contribution to journalArticlepeer-review

Abstract

The effect of pressure anisotropy on geomagnetic tail oscillations is studied using the Chew-Goldberger-Low equations. It is shown that anisotropy of the solar wind plasma pressure may result in generation of waves, assuming no waves in the case of isotropy. Anisotropy of the plasma pressure in the magnetospheric tail may also cause a basic distortion of the oscillation spectra.

Original languageEnglish
Pages (from-to)451-460
Number of pages10
JournalAstrophysics and Space Science
Volume21
Issue number2
DOIs
StatePublished - Apr 1973
Externally publishedYes

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