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An improved solution to the 'Rankine-Hugoniot' problemThis paper presents an extension of the nonlinear least squares fitting technique of Vinas and Scudder (1986) (VS), which finds the physical and geometrical properties of nondissipational magnetohydrodynamic (MHD) shocks. The new method incorporates plasma temperature observations in the form of normal momentum flux and energy density flux conservation as well as plasma density, velocity, and magnetic field data. The new technique is capable of using known standard deviations in the individual measurement points to properly weight the fitting procedure. The new fitting code is validated through the analysis of synthetic shocks with known physical and geometrical properties. Finally, it is compared to the original VS method and the preaveraged velocity coplanarity technique.
Document ID
19950053318
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Szabo, A.
(Massachusetts Institute of Technology, Cambridge, MA United States)
Date Acquired
August 16, 2013
Publication Date
August 1, 1994
Publication Information
Publication: Journal of Geophysical Research
Volume: 99
Issue: A8
ISSN: 0148-0227
Subject Category
Solar Physics
Report/Patent Number
ISSN: 0148-0227
Accession Number
95A84917
Funding Number(s)
CONTRACT_GRANT: JPL-957781
CONTRACT_GRANT: NAGW-2403
Distribution Limits
Public
Copyright
Other

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