Astronomy and Astrophysics – Astronomy
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.6511o&link_type=abstract
American Astronomical Society, 200th AAS Meeting, #65.11; Bulletin of the American Astronomical Society, Vol. 34, p.752
Astronomy and Astrophysics
Astronomy
1
Scientific paper
Recent advances in numerical methods and computer systems makes it possible to tackle complicated, more realistic dynamic phenomena appearing in the heliosphere. Representative simulations of large-scale structures require consideration of the preexisting structured ambient solar wind, realistic treatment of the launch of transient disturbances, and the consequent interaction of multiple ambient and transient structures. We will review recent progress in this area at NOAA/SEC, with special attention being given to the three- dimensional distortion of shocks and ICMEs (interplanetary counterparts of coronal mass ejections) propagating within the streamer belt and to effects generated during collisions of magnetic flux ropes and interplanetary shocks. Numerical results will be presented as evolving global structures as well as temporal profiles of plasma parameters at different observing points and line-of-sight images of light scattered from density structures.
Odstrcil Dusan
Pizzo Victor J.
No associations
LandOfFree
MHD Modeling of ICMEs 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 MHD Modeling of ICMEs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and MHD Modeling of ICMEs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1720025