Evolution of Flare Ribbons and Energy Release

Details Evolution of Flare Ribbons and Energy Release Evolution of Flare Ribbons and Energy Release

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3367a&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

We examined the relation between evolutions of flare ribb ons and released magnetic energies at a solar flare which occurred on 2001 April 10 in the active region NOAA 9415. We successfully evaluated the released energy quantitatively, based on the magnetic reconnection model. We measured the photospheric magnetic field strengths and the separation speeds of the fronts of the Hα flare ribb on, and estimated the released magnetic energy at the flare by using those values. Then, we compared the estimated energy release rates with the nonthermal behaviors observed in hard X-rays and microwaves. We found that those at the Hα kernels associated with the HXR sources are locally large enough to explain the difference between the spatial distribution the Hα kernels and the hard X-ray sources. Their temporal evolution of the energy release rates also shows peaks corresponding to hard X-ray bursts.

Affiliated with

Also associated with

No associations

Rating

Evolution of Flare Ribbons and Energy Release 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 Evolution of Flare Ribbons and Energy Release, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of Flare Ribbons and Energy Release will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1145639