Physics
Scientific paper
Sep 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..116..309k&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 116, no. 2, 1988, p. 309-321.
Physics
Angular Distribution, Electron Distribution, Electron Energy, Solar Flares, Solar X-Rays, Temporal Distribution, Bremsstrahlung, Electron Scattering, Gamma Ray Bursts, Monte Carlo Method
Scientific paper
Fine time variation of hard X-rays has been explained in terms of a spread in the angle of incidence of the source electrons in non-thermal thick-target model for bremsstrahlung generation. The electron energy and angular distributions have been calculated by combining small angle scatterings using analytical treatment with a large angle collision using Monte Carlo calculations as a function of column density. The computed X-ray pulse corresponds well with the observed fine time structure. The calculated spectra of X-rays at the peak and valley are also consistent with the observations.
Khosa P. N.
Koul Pradman K.
Rausaria R. R.
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