Solar neutrons and the energy spectrum of flare-accelerated particles

Details Solar neutrons and the energy spectrum of flare-accelerated particles Solar neutrons and the energy spectrum of flare-accelerated particles

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987izssr..51.1861k&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 51, Oct. 1987, p. 1861, 1862. In Russian.

Physics

Energy Spectra, Particle Acceleration, Solar Flares, Solar Neutrons, Angular Distribution, Magnetic Properties, Monte Carlo Method

Scientific paper

The Monte Carlo method is used to calculate the generation and escape of neutrons in the framework of the magnetic-arc model. It is shown that the generation of neutrons lasts for 20-30 minutes; the characteristic time of the intensity decline increases with magnetic field gradient and the radius of the coronal part of the arc. The angular distribution of escaping neutrons is anisotropic, with the maximum flux occurring at the limb. The neutron energy spectra are different in different directions. Particular attention is given to the solar-longitude dependence of neutron fluxes in a flare with gamma-ray emission.

Affiliated with

Also associated with

No associations

Rating

Solar neutrons and the energy spectrum of flare-accelerated particles 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 Solar neutrons and the energy spectrum of flare-accelerated particles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar neutrons and the energy spectrum of flare-accelerated particles will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1775609