Mean statistical structure of the magnetospheric tail according to satellite data

Details Mean statistical structure of the magnetospheric tail according to satellite data Mean statistical structure of the magnetospheric tail according to satellite data

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..987t&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Nov.-Dec. 1987, p. 987-993. In Russian.

Computer Science

1

Geomagnetic Tail, Magnetic Disturbances, Magnetospheric Instability, Plasma Layers, Satellite Observation, Approximation, Atmospheric Models

Scientific paper

Available satelite data are used to construct a quantitative model of magnetic-field distribution in the magnetotail and to investigate the dependence of the tail structure on the geomagnetic-disturbance level and solar-wind parameters. It is confirmed that the plasma sheet twists around the tail axis in a direction defined by the sign of the By component of the IMF. The penetration of the By component into the plasma sheeet and parts of the tail is investigated.

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