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The effect of Compton scattering on gamma-ray spectra of the 2005 January 20 flare

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The effect of Compton scattering on gamma-ray spectra of the 2005 January 20 flare

Research in Astron.Astrophys.2012 Vo1.12 No.10,1439—1450 http://www.raa-journa1.org http://www.iop.org/journals/raa Researchin Astronomyand Astrophysics The effect of Compton scattering on gamma-ray spectra of the 2005 January 20 flare Wei Chen and Wei—Qun Gan Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210008,China;w.[email protected].ac. Received 2012 March 23;accepted 2012 April 1 1 Abstract Gamma—ray spectroscopy provides a wealth of information about acceler- ated particles in solar flares,as well as the ambient medium with which these energetic particles interact.The neutron capture line(2.223 MeV),the strongest in the solar gamma—ray spectrum,forN1s in the deep atmosphere.The energy of these photons call be reduced via Compton scattering.With the fully relativistic GEANT4 toolkit,we have carried out Monte Carlo simulations of the transport of a neutron capture line in solar flares.and applied them to the flare that occ

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