Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...331.1029m&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 331, Aug. 15, 1988, p. 1029-1035.
Astronomy and Astrophysics
Astrophysics
25
Anisotropy, Gamma Ray Spectra, Particle Acceleration, Solar Corpuscular Radiation, Solar Flares, Spectrum Analysis, Alpha Particles, Angular Distribution, Beryllium Isotopes, Lithium, Solar Atmosphere
Scientific paper
The profiles of the 0.429 and 0.478 MeV gamma-ray lines from 7Be and 7Li (produced by interactions of flare-accelerated α-particles with ambient He in the solar atmosphere) and of the 4.438 MeV line from 12C (produced by inelastic scattering of 12C by accelerated protons) depend on the angular distribution of the interacting accelerated particles. The authors calculate the line profiles resulting from various assumed accelerated-particle angular distributions and show that it will be possible to distinguish among them using observations of gamma-ray spectra from solar flares obtained with high-resolution detectors.
Kozlovsky Benz
Murphy Ronald J.
Ramaty Reuven
No associations
LandOfFree
Gamma-ray spectroscopic tests for the anisotropy of accelerated particles in solar 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 Gamma-ray spectroscopic tests for the anisotropy of accelerated particles in solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-ray spectroscopic tests for the anisotropy of accelerated particles in solar flares will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1693695