Computer Science
Scientific paper
Apr 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..234t&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Mar.-Apr. 1989, p. 234-241. In Russian.
Computer Science
Earth Magnetosphere, Geomagnetism, Magnetospheric Instability, Night Sky, Space Plasmas, Adiabatic Conditions, Anisotropy, Magnetic Flux, Magnetic Storms
Scientific paper
The development of pressure anisotropy in the nighttime sector of the near magnetosphere is investigated in the adiabatic approximation. It is shown that a necessary condition for the development of an extended magnetic-field structure with a thin current sheet, characteristic of the end of the preliminary substorm phase, is the gradual decrease of the Bz component in the near-equatorial region. Attention is given to sources of the development of plasma anisotropy with p-parallel greater than o-perpendicular connected with azimuthal asymmetry of the magnetosphere.
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