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• W3100351978 endingPage "86" @default.
• W3100351978 startingPage "86" @default.
• W3100351978 abstract "Observations with {em RHESSI} have enabled the detailed study of the structure of dense hard X-ray coronal sources in solar flares. The variation of source extent with electron energy has been discussed in the context of streaming of non-thermal particles in a one-dimensional cold-target model, and the results used to constrain both the physical extent of, and density within, the electron acceleration region. Here we extend this investigation to a more physically realistic model of electron transport that takes into account the finite temperature of the ambient plasma, the initial pitch-angle distribution of the accelerated electrons, and the effects of collisional pitch-angle scattering. The finite temperature results in the thermal diffusion of electrons, that leads to the observationally-inferred value of the acceleration region volume being an overestimate of its true value. The different directions of the electron trajectories, a consequence of both the non-zero injection pitch-angle and scattering within the target, cause the projected propagation distance parallel to the guiding magnetic field to be reduced, so that a one-dimensional interpretation can overestimate the actual density by a factor of up to $sim 6$. The implications of these results for the determination of acceleration region properties (specific acceleration rate, filling factor, etc.) are discussed." @default.
• W3100351978 created "2020-11-23" @default.
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• W3100351978 date "2014-05-06" @default.
• W3100351978 modified "2023-10-18" @default.
• W3100351978 title "ON THE VARIATION OF SOLAR FLARE CORONAL X-RAY SOURCE SIZES WITH ENERGY" @default.
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• W3100351978 doi "https://doi.org/10.1088/0004-637x/787/1/86" @default.
• W3100351978 hasPublicationYear "2014" @default.
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