The Magnetic Structure of CR1922

Details The Magnetic Structure of CR1922 The Magnetic Structure of CR1922

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh42b0520l&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH42B-0520

Physics

7509 Corona

Scientific paper

The May 12, 1997 halo CME occurred during CR 1922, when the state of the sun was quiet. The CME is associated with decaying active region AR 8038. It was the only active center on the disk and was the sight for flaring activity for several day surrounding the CME. This event has gained great interest lately due to the wide range of observations made before, during and after the event. It has been selected by several groups as an example of a real event that they will try to simulate. We examine the magnetic structure of the solar corona during this Carrington rotation using a synoptic map driven MHD model of the solar corona.

Affiliated with

Also associated with

No associations

Rating

The Magnetic Structure of CR1922 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 The Magnetic Structure of CR1922, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Magnetic Structure of CR1922 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1647033