The magnetic geometry and structure of the giant post-flare arch of 21-22 May, 1980

Details The magnetic geometry and structure of the giant post-flare arch of 21-22 May, 1980 The magnetic geometry and structure of the giant post-flare arch of 21-22 May, 1980

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116..163p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 116, no. 1, 1988, p. 163-178. NASA-CNR-supported research.

Physics

21

Particle Acceleration, Relativistic Velocity, Solar Electrons, Solar Flares, Solar Protons, Shock Wave Propagation, Solar Magnetic Field

Scientific paper

The authors use the observed photospheric line-of-sight magnetic field distribution to compute, in the current-free approximation, the three-dimensional topology of the coronal field above the flare site. Comparing the HXIS intensity contours of the arch to the projected shapes of the field lines suggests that the arch is indeed aligned with certain coronal flux tubes and allows an independent determination of the geometrical arch parameters to be made. The results suggest that the arch may be a by-product of magnetic reconnection occurring far above the flare site.

Affiliated with

Also associated with

No associations

Rating

The magnetic geometry and structure of the giant post-flare arch of 21-22 May, 1980 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 magnetic geometry and structure of the giant post-flare arch of 21-22 May, 1980, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The magnetic geometry and structure of the giant post-flare arch of 21-22 May, 1980 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1693142