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Interplanetary shock normalsA scheme has been developed to improve the estimate of an interplanetary shock normal by using both magnetic field and plasma data from a single spacecraft. Calculation of the basic shock model employs a subset of the eight magnetohydrodynamic conservation relations for a shock in an isotropic medium. This subset consists of six equations that are devoid of pressure and temperature terms. A sigma-weighted least squares loss function technique is used to best fit the overdetermination equations with respect to the eleven parameters of the system. This procedure usually yields a normal much more accurate than the one obtained using magnetic field values alone. An example is given of the use of the technique on the data for the Pioneer 7 shock of 29 August 1966.
Document ID
19720015699
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lepping, R. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 6, 2013
Publication Date
January 1, 1972
Publication Information
Publication: Significant Accomplishments in Sci., 1970
Subject Category
Space Sciences
Accession Number
72N23349
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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