Ion and relativistic electron transport in solar flares

Details Ion and relativistic electron transport in solar flares Ion and relativistic electron transport in solar flares

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...73..199r&link_type=abstract

(NASA and University of New Hampshire, Workshop on Impulsive Solar Flares, 2nd, Durham, NH, Sept. 26-28, 1988) Astrophysical Jou

Astronomy and Astrophysics

Astrophysics

13

Gamma Ray Bursts, Ion Beams, Relativistic Electron Beams, Solar Flares, Bremsstrahlung, Emission Spectra, Gamma Ray Spectra, Monte Carlo Method, Particle Acceleration, Solar Magnetic Field, Transport Properties

Scientific paper

Recent models for the ion and relativistic electron transport in solar flare magnetic loops are reviewed, focusing on the ways in which the models handle loop structure, particle acceleration, and particle transport. Results are presented from Monte Carlo simulations of ion and relativistic ion transport. Consideration is given to results concerning the depth distributions of gamma-ray production, the attenuation of gamma-ray lines, the time dependences of the various emissions and the angular distribution of the bremsstrahlung.

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