Quiescent prominences - Where are they formed?

Details Quiescent prominences - Where are they formed? Quiescent prominences - Where are they formed?

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..107..233t&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 107, no. 2, 1987, p. 233-237.

Physics

49

Magnetic Field Configurations, Solar Atmosphere, Solar Flares, Solar Prominences, H Alpha Line, Solar Activity, Solar Cycles, Stellar Mass Ejection

Scientific paper

An investigation of two years of quiescent prominences shows that substantially more (20 percent in 1973 and 96 percent in 1979) quiescent prominences were formed on neutral lines between bipolar regions than on neutral lines inside bipolar regions. An examination of the associated solar activity of the seven white light coronal transients observed by Skyklab indicates that regardless of where the prominences were formed, their eruptions can cause observable coronal mass ejections. The present results suggest that a prominence model is needed in which the evolution begins at the boundary of two adjacent bipolar regions.

Affiliated with

Also associated with

No associations

Rating

Quiescent prominences - Where are they formed? 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 Quiescent prominences - Where are they formed?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Quiescent prominences - Where are they formed? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1761855