Mathematics – Logic
Scientific paper
Jul 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983chjss...3r.177c&link_type=abstract
Chinese Journal of Space Science, vol. 3, July 1983, p. 177-183. In Chinese, with abstract in English.
Mathematics
Logic
1
Astronomical Models, Solar Flares, Solar Prominences, Chromosphere, Filaments, Magnetic Field Configurations, Morphology, Solar Magnetic Field
Scientific paper
Data from 20 spotless flares observed during the peak period of solar cycle 21 and from two major spotless two-ribbon flares have been analyzed, and the morphological features of the flares are reported. These features are then qualitatively explained on the basis of the Kippenhahn-Schlueter filament model. From calculated results for the magnetic energy, it is concluded that the free energy stored in the sheared field surrounding a quiescent filament can be as great as the energy released in a middle flare occurring in the active region. In accordance with the coronal current equilibrium model of Van Tend and Kuperus (1978), the force caused by nonequilibrium can cause the filament current to rise and reach a new equilibrium state when the filament current exceeds the local limit of the current.
Cao Tian-Jun
Chen Li-Chyong
Luo Bao-Rong
Xu Aiguo
Zhi Z.-X.
No associations
LandOfFree
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.
Profile ID: LFWR-SCP-O-1627423