ELF emissions observed by the EXOS-D satellite around the geomagnetic equatorial region

Details ELF emissions observed by the EXOS-D satellite around the geomagnetic equatorial region ELF emissions observed by the EXOS-D satellite around the geomagnetic equatorial region

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991georl..18..317s&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 18, Feb. 1991, p. 317-320.

Physics

6

Equatorial Regions, Exos Satellites, Exos-D Satellite, Extremely Low Radio Frequencies, Geomagnetism, Helium Ions, Ion Cyclotron Radiation, Magnetic Field Configurations, Oxygen Ions, Ray Tracing

Scientific paper

The mechanism responsible for the equatorial-region ELF emission detected by the Japanese EXOS-D satellite and reported by Kimura et al. (1990) is considered theoretically. Typical data are presented in graphs and sample spectra and discussed in detail. Since the emission frequencies were above the cyclotron frequencies of He(+) and O(+), it is proposed that they are ion-cyclotron emissions trapped along the magnetic-field lines, as observed previously by GEOS 1 and 2 and reported by Young et al. (1981) and Roux et al. (1982).

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