Physics
Scientific paper
Jan 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..125...67k&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 125, Jan. 1990, p. 67-90.
Physics
12
Coronal Loops, Neutron Emission, Solar Flares, Gamma Ray Spectra, High Energy Electrons, Solar Radiation
Scientific paper
Secondaries produced by accelerated particles trapped in a coronal magnetic structure as well as by those precipitating down into dense regions of the solar atmosphere are considered. Time profiles and generation anisotropy for pi(0) decay gamma-radiaton, nuclear gamma-ray lines, and greater than 10 MeV electron bremsstrahlung in a flare magnetic arch. It is shown that as primary particles move inside a magnetic arch in an inhomogeneous atmosphere the secondary emission turns out to be anisotropical, even if the acceleration process is an isotropical one. On the other hand, the anisotropy of the acceleration process not only influences the directivity of secondary emission but also its intensity decay rate. The exact as well as the simple approximate calculation techniques for the angular and temporal characteristics of gamma-ray emission are discussed.
Kocharov Leon G.
Koval'Tsov G. A.
No associations
LandOfFree
Generation of high-energy neutral radiation in flare loops. I -Basic regularities 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 Generation of high-energy neutral radiation in flare loops. I -Basic regularities, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Generation of high-energy neutral radiation in flare loops. I -Basic regularities will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1565300