Non-thermal particles in the solar atmosphere during flare developments and in the absence of flares

Details Non-thermal particles in the solar atmosphere during flare developments and in the absence of flares Non-thermal particles in the solar atmosphere during flare developments and in the absence of flares

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..221v&link_type=abstract

Advances in Space Research, Volume 13, Issue 9, p. 221-231.

Physics

6

Scientific paper

Non-thermal particles play a major role in the active Sun since they contain a large amount of the energy released during flares and since dekakeV electrons are produced in the absence of flares in association with active regions. These particles are detected either in the interplanetary space or through the radiations they produce in the solar atmosphere during flares (radio, X-ray/γ-ray bursts) and outside flares (e.g. radio noise storms). We focus on the particles interacting at the Sun. After a brief discussion on emission processes, we discuss some evidences for the fragmentation of the non- thermal energy release during flares and present some observations relevant to the onset of noise storms. New results obtained on the more energetic flares are then summarized: relative amount of accelerated electrons and ions, particle transport from the acceleration site to the emitting regions, hard X-ray and γ-ray coronal contributions from partially trapped particles, high energy (>= 10 MeV) radiation from relativistic electrons and 100 MeV-1 GeV ions.

Affiliated with

Also associated with

No associations

Rating

Non-thermal particles in the solar atmosphere during flare developments and in the absence of flares 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 Non-thermal particles in the solar atmosphere during flare developments and in the absence of flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-thermal particles in the solar atmosphere during flare developments and in the absence of flares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1559415