Coupled MHD-Inner Magnetosphere Simulations of Geomagnetic Storms

Details Coupled MHD-Inner Magnetosphere Simulations of Geomagnetic Storms Coupled MHD-Inner Magnetosphere Simulations of Geomagnetic Storms

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sm32a02d&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SM32A-02

Statistics

Computation

2431 Ionosphere/Magnetosphere Interactions (2736), 2730 Magnetosphere--Inner, 2736 Magnetosphere/Ionosphere Interactions, 2788 Storms And Substorms

Scientific paper

The adaptive-grid Michigan MHD model (BATSRUS) has been coupled to a new high Rice Convection Model (RCM). This fully coupled code gives the possibility to realistically undertake global MHD simulations of a magnetic storm and the computation of both Region 1 and Region 2 currents. We will review details of the two models and their coupling, and report on the results of our first storm time simulation with the coupled code and show a comparison with observations. We will discuss the global observations provided by arrays of magnetometers which measure the temporal and spatial development of the ring current as well as high latitude global electrodynamic parameters derived from the AMIE and LiMIE data inversion techniques.

Affiliated with

Also associated with

No associations

Rating

Coupled MHD-Inner Magnetosphere Simulations of Geomagnetic Storms 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 Coupled MHD-Inner Magnetosphere Simulations of Geomagnetic Storms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coupled MHD-Inner Magnetosphere Simulations of Geomagnetic Storms will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1277129