Computer simulation of the dynamics of the near-earth part of the geomagnetic tail

Details Computer simulation of the dynamics of the near-earth part of the geomagnetic tail Computer simulation of the dynamics of the near-earth part of the geomagnetic tail

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ruht.rept.....w&link_type=abstract

Final Report, 1 Jan. 1983 - 4 May 1986 Rice Univ., Houston, TX. Dept. of Space Physics and Astronomy.

Physics

Space Physics

Computerized Simulation, Dynamic Models, Earth (Planet), Earth Magnetosphere, Geomagnetic Tail, Coding, Convection, Geomagnetism, Low Altitude, Magnetic Storms, Magnetohydrodynamics

Scientific paper

The objective of the contract was to extend the Rice Convection Modeling capabilities tailward to include the near Earth part of the geomagnetic tail, in order to include the dynamics of that region in our substorm simulations. The effort was divided into three parts: (1) development of equilibrium magnetic-field models; (2) development of an MHD code for use in the near magnetotail for periods when flows are supersonic or super-Alfvenic; and (3) modification of the Rice Convection Model to make it applicable further out in the magnetotail.

Affiliated with

Also associated with

No associations

Rating

Computer simulation of the dynamics of the near-earth part of the geomagnetic tail 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 Computer simulation of the dynamics of the near-earth part of the geomagnetic tail, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Computer simulation of the dynamics of the near-earth part of the geomagnetic tail will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1776081