An observational evidence of the flare model related to filament currents

Details An observational evidence of the flare model related to filament currents An observational evidence of the flare model related to filament currents

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acasn..32..343x&link_type=abstract

(Acta Astronomica Sinica, vol. 32, no. 4, 1991, p. 343-352) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 16, no. 2,

Astronomy and Astrophysics

Astrophysics

1

Magnetic Field Configurations, Solar Flares, Solar Magnetic Field, Solar Prominences, Astronomical Models, Equations Of Motion, Solar Activity, Solar X-Rays

Scientific paper

By analyzing the observed data about the impulsive phase of four flares and the regularities of motions of the relevant filaments, it is demonstrated quantitatively that the increase of the filament currents and the rapid motion of the filament are an indication of the occurrence of flares. The moment of the beginning of the impulsive phase is consistent with that of the maximum of the filament energy. Results show that the flare energy is supplied by the filament.

Affiliated with

Also associated with

No associations

Rating

An observational evidence of the flare model related to filament currents 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 An observational evidence of the flare model related to filament currents, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An observational evidence of the flare model related to filament currents will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1536369