A review of the October 21, 1989 red aurora seen in Japan and from the AKEBONO (EXOS-D) satellite.

Details A review of the October 21, 1989 red aurora seen in Japan and from the AKEBONO (EXOS-D) satellite. A review of the October 21, 1989 red aurora seen in Japan and from the AKEBONO (EXOS-D) satellite.

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992cajph..70..488.&link_type=abstract

Can. J. Phys., Vol. 70, No. 7, p. 488 - 499

Physics

2

Scientific paper

Observations of the October 21, 1989 red aurora from the ground and AKEBONO satellite are reviewed. Electric-field fluctuations associated with the auroral oval during the observation, together with auroral green-rayed structures embedded in the red veil strongly suggest that some electron acceleration mechanism was operative in the particle precipitation. Therefore this was not a typical stable auroral red (SAR) arc. This red aurora was most likely located at a low-latitude portion of an expansion aurora during an auroral substorm.

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