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Nonlocal plasma turbulence associated with interplanetary shocksRegions of plasma turbulence extending several tenths of an astronomical unit upstream or downstream of interplanetary shocks have been detected by the plasma wave instrument on ISEE 3. Highly impulsive electric field bursts at 1-10 kHz were found (hours upstream of quasi-parallel interplanetary shocks) whose average and peak amplitudes occasionally increased until the shock crossing, when they were suppressed. A 0.1-1 kHz electric field component was enhanced at nearly all shocks, and persisted downstream. A smooth, high-frequency continuum near and above the local electron plasma frequency was enhanced at, and persisted downstream of, every interplanetary shock studied. While no single interplanetary shock showed every effect, the ensemble of shocks contained at least one example of each type of plasma wave found upstream of the earth's bow shock.
Document ID
19820036543
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kennel, C. F.
(TRW Defense and Space Systems Group Redondo Beach, CA, United States)
Coroniti, F. V.
(TRW Defense and Space Systems Group, Redondo Beach; California, University Los Angeles, CA, United States)
Scarf, F. L.
(TRW Defense and Space Systems Group Redondo Beach, CA, United States)
Smith, E. J.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Gurnett, D. A.
(Iowa, University Iowa City, IA, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: Journal of Geophysical Research
Volume: 87
Subject Category
Astrophysics
Accession Number
82A20078
Funding Number(s)
CONTRACT_GRANT: NAS5-20093
CONTRACT_GRANT: NAS5-20682
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: NGL-16-001-043
Distribution Limits
Public
Copyright
Other

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