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August 1972 solar-terrestrial events - Observations of interplanetary shocks at 2.2 AUSimultaneous magnetic field and plasma observations on Pioneer 10 were used to identify three shocks and a plasma driver (possible flare ejecta) at 2.2 AU caused by the four large solar flares of August 2-7, 1972. Two shocks, the first and third, were forward shocks, while the second was a reverse shock. The local inertial velocities of all three shocks were estimated under the assumption of quasi-perpendicularity, i.e., the shocks were assumed to be propagating principally across, rather than along, the interplanetary magnetic field.
Document ID
19770044461
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Smith, E. J.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Davis, L., Jr.
(California Institute of Technology Pasadena, Calif., United States)
Coleman, P. J., Jr.
(California, University Los Angeles, Calif., United States)
Colburn, D. S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Dyal, P.
(NASA Ames Research Center Moffett Field, Calif., United States)
Jones, D. E.
(Brigham Young University Provo, Utah, United States)
Date Acquired
August 8, 2013
Publication Date
March 1, 1977
Publication Information
Publication: Journal of Geophysical Research
Volume: 82
Subject Category
Solar Physics
Accession Number
77A27313
Funding Number(s)
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: NGR-05-002-160
Distribution Limits
Public
Copyright
Other

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