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Interplanetary magnetic field enhancements in the solar wind Statistical properties at 1 AUThe present investigation is concerned with interplanetary magnetic field (IMF) enhancements which do not resemble any of the previously reported amplifications in the IMF. The magnetic field enhacements observed increase slowly at first and then more rapidly to a peak followed by a symmetrical decay. Interplanetary magnetic field enhacement observed by ISEE-3 on various dates are considered, giving attention to observations on June 5, 1979; September 8-9, 1980; February 5, 1981; and June 14-15, 1981. Interplanetary magnetic field enhancement observed with the aid of IMP-8 are also considered. A total of 45 events is found in surveying a 9-year period of magnetic field data.
Document ID
19850056134
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Arghavani, M. R.
(California Univ. Los Angeles, CA, United States)
Russell, C. T.
(California Univ. Los Angeles, CA, United States)
Luhmann, J. G.
(California Univ. Los Angeles, CA, United States)
Elphic, R. C.
(California, University Los Angeles, CA, United States)
Date Acquired
August 12, 2013
Publication Date
May 1, 1985
Publication Information
Publication: Icarus
Volume: 62
ISSN: 0019-1035
Subject Category
Solar Physics
Accession Number
85A38285
Funding Number(s)
CONTRACT_GRANT: NAS5-25771
CONTRACT_GRANT: NAGW-717
Distribution Limits
Public
Copyright
Other

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