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Fast and optimal solution to the 'Rankine-Hugoniot problem'A new, definitive, reliable and fast iterative method is described for determining the geometrical properties of a shock (i.e., theta sub Bn, yields N, V sub s and M sub A), the conservation constants and the self-consistent asymptotic magnetofluid variables, that uses the three dimensional magnetic field and plasma observations. The method is well conditioned and reliable at all theta sub Bn angles regardless of the shock strength or geometry. Explicit proof of uniqueness of the shock geometry solution by either analytical or graphical methods is given. The method is applied to synthetic and real shocks, including a bow shock event and the results are then compared with those determined by preaveraging methods and other iterative schemes. A complete analysis of the confidence region and error bounds of the solution is also presented.
Document ID
19860037041
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Vinas, A. F.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Scudder, J. D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1986
Publication Information
Publication: Journal of Geophysical Research
Volume: 91
ISSN: 0148-0227
Subject Category
Astrophysics
Accession Number
86A21779
Distribution Limits
Public
Copyright
Other

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