Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions

Details Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ge%26ae..50..303b&link_type=abstract

Geomagnetism and Aeronomy, Volume 50, Issue 3, pp.303-313

Physics

1

Scientific paper

The initial parameters of disturbing fluxes of coronal mass ejections (CMEs) such as loop, front, spike, multiple structure ejection, and structureless ejection, which cannot be determined from direct observations, are determined using the data on the interplanetary coronal mass ejections (ICMEs) registered on the Helios and Pioneer Venus Orbiter spacecraft in the vicinity of Venus. The method of MHD modeling the modified initial parameters of CMEs has been used for this purpose. The ICME parameters have been analyzed in order to determine the types of the solar sources of the considered plasma flows.

Affiliated with

Also associated with

No associations

Rating

Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions 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 Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1829502