Three-point magnetic field observations of substorms in the inner magnetotail

Details Three-point magnetic field observations of substorms in the inner magnetotail Three-point magnetic field observations of substorms in the inner magnetotail

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94.3565f&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 94, April 1, 1989, p. 3565-3578.

Computer Science

Sound

16

Geomagnetic Tail, Geomagnetism, Magnetic Storms, Satellite Sounding, Equatorial Atmosphere, Goes Satellites, Magnetic Signatures, Night Sky, Space Plasmas

Scientific paper

Three-point AMPTE/CCE and GOES 5 and 6 magnetic field observations of substorms in the inner magnetotail, provided by the AMPTE/CC, GOES 5, and GOES 6 satellites, were used to investigate the magnetotail changes as a function of radial distance and latitude. Data analysis indicates that observed phenomena depend significantly on these two coordinates. The results were, in general, consistent with the current wedge concept of Nagai (1987).

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