Statistics – Computation
Scientific paper
May 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986stin...8630621s&link_type=abstract
Unknown
Statistics
Computation
Comets, Mathematical Models, Solar Planetary Interactions, Solar Wind, Three Dimensional Bodies, Three Dimensional Models, Magnetohydrodynamic Waves, Plasma Interactions, Supersonic Flow
Scientific paper
This is the final summary report by Resource Management Associates, Inc., of the first year's work under Contract No. NASW-4011 to the National Aeronautics and Space Administration. The work under this initial phase of the contract relates to the preliminary development of a global, 3-D magnetohydrodynamic computational model to quantitatively describe the detailed continuum field and plasma interaction process of the solar wind with cometary and planetary bodies throughout the solar system. The work extends a highly-successful, observationally-verified computational model previously developed by the author, and is appropriate for the global determination of supersonic, super-Alfvenic solar wind flows past planetary obstacles. This report provides a concise description of the problems studied, a summary of all the important research results, and copies of the publications.
No associations
LandOfFree
Preliminary development of a global 3-D magnetohydrodynamic computational model for solar wind-cometary and planetary interactions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Preliminary development of a global 3-D magnetohydrodynamic computational model for solar wind-cometary and planetary interactions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Preliminary development of a global 3-D magnetohydrodynamic computational model for solar wind-cometary and planetary interactions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1776896