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Rocket observations of energetic particles at the geomagnetic equatorEnergetic particle detectors were included in the payloads of two rockets launched in Peru during the Condor campaign of 1983. These night-time flights reached altitudes of 587 and 535 km, respectively. The pitch-angle distribution is anisotropic with the maximum at 90 deg. Each payload included two solid-state detectors differing in the thickness of the aluminum coating. Comparison of the fluxes measured by the two detectors leads to the conclusion that, on both occasions, the energetic particles are predominantly helium ions. The flux is small below 200 km, increases linearly to 350 km, and then more slowly to apogee. The east-west asymmetry of flux, noted at 200 km in a previous equatorial launch, is not seen at greater altitudes, consistent with the flux profile and the large gyroradius of the ions.
Document ID
19860034345
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Smith, L. G.
(Illinois Univ. Urbana, IL, United States)
Houshmand, B.
(Illinois, University Urbana, United States)
Date Acquired
August 12, 2013
Publication Date
October 1, 1985
Publication Information
Publication: Journal of Atmospheric and Terrestrial Physics
Volume: 47
ISSN: 0021-9169
Subject Category
Geophysics
Accession Number
86A19083
Funding Number(s)
CONTRACT_GRANT: NGR-14-005-181
Distribution Limits
Public
Copyright
Other

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