The 4 February, 1986 flare and flare-filament current model.

Details The 4 February, 1986 flare and flare-filament current model. The 4 February, 1986 flare and flare-filament current model.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..163..133t&link_type=abstract

Solar Physics, Vol. 163, No. 1, p. 133 - 144

Physics

4

Solar Flares: Currents, Solar Flares: H Alpha, Solar Flares: Multiwavelength Observations, Solar Flares: Models

Scientific paper

The observational data in Hα, radio, soft X-ray, hard X-ray, and γ-ray emissions for the 3B/X3.0 solar flare on 4 February, 1986 are collected. This flare is studied in detail by using the flare-filament current model. The momentum equations and the energy equations of the filament current have been solved. The influence of the highly sheared background magnetic field on the motion of the filaments is studied through numerical calculation. The results show that the resistive tearing instability is a possible pre-heating mechanism in the preflare phase, and both the rotation of the spiral sunspots and the highly sheared background field are necessary for the energy storage of this flare. The high-energy data of the flare imply that the current-loop coalescence instability is a possible eruptive mechanism.

Affiliated with

Also associated with

No associations

Rating

The 4 February, 1986 flare and flare-filament current 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 The 4 February, 1986 flare and flare-filament current model., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 4 February, 1986 flare and flare-filament current model. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1129979