NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Numerical experimentation on spherically symmetric one-dimensional magnetohydrodynamic /MHD/ wave propagationRadial propagation of one-dimensional magnetohydrodynamic (MHD) waves are analyzed numerically on the basis of the Implicit-Continuous-Fluid-Eulerian (ICE) scheme. Accuracy of the numerical method and other properties are tested through the study of MHD wave propagation. The three different modes of MHD waves (i.e., fast-, slow- and Alfven (transverse) mode) are generated by applying physically consistent boundary perturbations derived from MHD compatibility relations. It is shown that the resulting flow following these waves depend upon the relative configurations of the initial magnetic field and boundary perturbations.
Document ID
19820050324
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Han, S. M.
(Alabama Univ. Huntsville, AL, United States)
Wu, S. T.
(Alabama Univ. Huntsville, AL, United States)
Nakagawa, Y.
(Alabama, University Huntsville, AL, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: Computers and Fluids
Volume: 10
Issue: 3, 19
Subject Category
Plasma Physics
Accession Number
82A33859
Funding Number(s)
CONTRACT_GRANT: NSF ATM-77-22484
CONTRACT_GRANT: NAGW-9
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available