Statistics – Computation
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..527v&link_type=abstract
In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2
Statistics
Computation
Coronal Mass Ejections, Modeling, Mhd Simulations
Scientific paper
Coronal mass ejections (CMEs) are transient expulsions of solar plasma from the gravitational field of the Sun as seen in white light coronagraph observations. Their interplanetary manifestations are called interplanetary coronal mass ejections (ICMEs). This review deals with ICMEs from a theoretical point of view. During recent years a significant progress in numerical modeling of ICMEs has been achieved. This is caused by increasing power of computational resources, which enables to perform three dimensional magnetohydrodynamic simulations. These simulations of ICME evolution help us to better understand observations of interplanetary transient events. And the same is true for various analytical or semi-analytical models of ICMEs, which are also briefly described.
No associations
LandOfFree
Interplanetary 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 Interplanetary modeling of ICMEs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interplanetary modeling of ICMEs will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1152896