Coronal Mass Ejections and Eruptive Prominences: Mutual Spatial Arrangement

Details Coronal Mass Ejections and Eruptive Prominences: Mutual Spatial Arrangement Coronal Mass Ejections and Eruptive Prominences: Mutual Spatial Arrangement

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004arep...48..145l&link_type=abstract

Astronomy Reports, vol. 48, Issue 2, p.145-152

Astronomy and Astrophysics

Astronomy

Scientific paper

The mutual spatial arrangement of coronal mass ejections and eruptive prominences on the Sun is considered. These phenomena occur on different scales and are observed at different heights above the solar surface. In spite of the presumed causal connection between them, they are often widely separated in position angle at epochs of solar minimum. This means that the motion of a prominence in the corona is not strictly radial and has an appreciable component along the surface. This behavior can be explained in a model of a filament as a magnetic flux rope in equilibrium in the coronal magnetic field. The initial trajectory of the filament is determined by the structure of the global field.

Affiliated with

Also associated with

No associations

Rating

Coronal Mass Ejections and Eruptive Prominences: Mutual Spatial Arrangement 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 Coronal Mass Ejections and Eruptive Prominences: Mutual Spatial Arrangement, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal Mass Ejections and Eruptive Prominences: Mutual Spatial Arrangement will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1602436