Actions for MHD Modeling of the Interaction of the Solar Wind With Venus

Email RIS file
Bookmark
Report an Issue

MHD Modeling of the Interaction of the Solar Wind With Venus

Author
Steinolfson, R. S.
Published
Oct. 25, 1996.
Physical Description
1 electronic document
Online Version

Availability

I Want It
I Want It

Finding items...

Restrictions on Access
Unclassified, Unlimited, Publicly available.
Free-to-read Unrestricted online access
Summary
The primary objective of this research program is to improve our understanding of the physical processes occurring in the interaction of the solar wind with Venus. This will be accomplished through the use of numerical solutions of the two- and three-dimensional magnetohydrodynamic (MHD) equations and through comparisons of the computed results with available observations. A large portion of this effort involves the study of processes due to the presence of the magnetic field and the effects of mass loading. Published papers are included in the appendix.
Other Subject(s)
Collection
NASA Technical Reports Server (NTRS) Collection.
Note
Document ID: 19970002922.
Accession ID: 97N11710.
NAS 1.26:202519.
NASA-CR-202519.
Terms of Use and Reproduction
No Copyright.
View MARC record | catkey: 15649255