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The interplanetary shock event of November 11/12 1978 - A comprehensive test of acceleration theoryA comprehensive study of the November 11, 12, 1978 shock event based on energetic particle, solar wind, magnetic field and wave data from the ISEE-3, -1 and -2 spacecraft has been undertaken both from the energetic and the collisionless shock point of view. The energy density of 10-50 keV protons accelerated by the shock is found to be equivalent to the upstream magnetic field energy density. The observations are in quantitative agreement with Lee's (1983) self consistent theory for the excitation of hydromagnetic waves and the acceleration of ions upstream of interplanetary shocks.
Document ID
19850040707
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Wenzel, K.-P.
(California Univ. Los Angeles, CA, United States)
Sanderson, T. R.
(California Univ. Los Angeles, CA, United States)
Van Nes, P.
(ESA Space Science Dept., Noordwijk, Netherlands)
Kennel, C. F.
(California Univ. Los Angeles, CA, United States)
Scarf, F. L.
(California Univ. Los Angeles, CA, United States)
Coroniti, F. V.
(TRW Space and Technology Group Redondo Beach, CA, United States)
Russell, C. T.
(California, University Los Angeles, CA, United States)
Parks, G. K.
(Washington, University Seattle, WA, United States)
Smith, E. J.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena CA, United States)
Feldman, W. C.
(Los Alamos National Laboratory Los Alamos, NM, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1983
Subject Category
Astrophysics
Meeting Information
Meeting: International Cosmic Ray Conference
Location: Bangalore
Country: India
Start Date: August 22, 1983
End Date: September 3, 1983
Accession Number
85A22858
Distribution Limits
Public
Copyright
Other

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