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Energetic particle activity at 5-min and 10-s time resolution in the magnetotail and its relation to auroral activityThe paper examines several energetic particle bursts associated with substorm events in the magnetotail using data from the Imp 7 and 8 spacecraft experiments. Individual proton and electron bursts observed by the spacecraft do not always coincide nor does magnetotail activity correlate strongly with auroral activity on time scales less than 1 hr. The pitch angle distributions were determined with a time resolution of 10 s by combining magnetic field and particle measurements on Imp 8; during intense particle bursts the 0.3-MeV protons exhibit unidirectional or bidirectional anisotropies along the magnetic field. The data suggest the presence of small localized acceleration regions in the magnetotail observable when magnetically connected to the spacecraft; little evidence is found for a single neutral line extending across the width of the magnetotail.
Document ID
19800036997
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Carbary, J. F.
(Johns Hopkins Univ. Silver Spring, MD, United States)
Krimigis, S. M.
(Johns Hopkins University Applied Physics Laboratory, Laurel, Md., United States)
Date Acquired
August 10, 2013
Publication Date
December 1, 1979
Publication Information
Publication: Journal of Geophysical Research
Volume: 84
Subject Category
Geophysics
Accession Number
80A21167
Funding Number(s)
CONTRACT_GRANT: NASA TASK I
CONTRACT_GRANT: N00024-78-C-5384
CONTRACT_GRANT: NSF ATM-76-81099
Distribution Limits
Public
Copyright
Other

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