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On the standing wave mode of giant pulsationsIn order to determine the standing wave mode of giant pulsations, a systematic survey of magnetic field data from the AMPTE CCE spacecraft and from ground stations located near the geomagnetic foot point of CCE was made. One giant pulsation was associated with a compressional wave, while no giant pulsation was observed in association with transverse wave events. The CCE magnetic field record for the giant pulsation exhibited a remarkable similarity to a giant pulsation observed from the ATS 6 geostationary satellite near the magnetic equator. It is concluded that the compressional nature of the giant pulsation is due to an odd-mode standing wave structure, which places a strong constraint on the generation mechanism of giant pulsations.
Document ID
19920064846
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Takahashi, K.
(Johns Hopkins University Laurel, MD, United States)
Sato, N.
(National Institute of Polar Research Tokyo, Japan)
Warnecke, J.
(NASA Headquarters Washington, DC United States)
Luehr, H.
(Braunschweig, Technische Universitaet Federal Republic of Germany, United States)
Spence, H. E.
(Aerospace Corp., Space and Environment Technology Center El Segundo, CA, United States)
Tonegawa, Y.
(Tokai University Hiratsuka, Japan)
Date Acquired
August 15, 2013
Publication Date
July 1, 1992
Publication Information
Publication: Journal of Geophysical Research
Volume: 97
Issue: A7 J
ISSN: 0148-0227
Subject Category
Geophysics
Accession Number
92A47470
Funding Number(s)
CONTRACT_GRANT: N00039-89-C-5301
CONTRACT_GRANT: F04701-88-C-0089
Distribution Limits
Public
Copyright
Other

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