Morphological features of spotless flares and a possible theoretical model

Details Morphological features of spotless flares and a possible theoretical model Morphological features of spotless flares and a possible theoretical model

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983chjss...3q.177c&link_type=abstract

(Chinese Journal of Space Science, vol. 3, no. 3, 1983, p. 177-183) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 7,

Astronomy and Astrophysics

Astrophysics

Magnetic Field Configurations, Solar Flares, Solar Magnetic Field, Stellar Models, Energy Sources, Filaments, Morphology, Solar Prominences, Taylor Instability

Scientific paper

The morphological features of spotless flares as observed by three Chinese observatories (Yunnan, Purple Mountain, and Beijing) during the peak years of the 21st solar cycle are summarized. On the basis of the Kippenhahn-Schlueter model of solar prominences, these observed features are qualitatively interpreted and a possible theoretical model of generating spotless flares is proposed.

Affiliated with

Also associated with

No associations

Rating

Morphological features of spotless flares and a possible theoretical model 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 Morphological features of spotless flares and a possible theoretical model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Morphological features of spotless flares and a possible theoretical model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1802982