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• W3098895887 startingPage "A64" @default.
• W3098895887 abstract "The imaging spectroscopy capabilities of the Reuven Ramaty high energy solar spectroscopic imager (RHESSI) enable the examination of the accelerated electron distribution throughout a solar flare region. In particular, it has been revealed that the energisation of these particles takes place over a region of finite size, sometimes resolved by RHESSI observations. In this paper, we present, for the first time, a spatially distributed acceleration model and investigate the role of inhomogeneous acceleration on the observed X-ray emission properties. We have modelled transport explicitly examining scatter-free and diffusive transport within the acceleration region and compare with the analytic leaky-box solution. The results show the importance of including this spatial variation when modelling electron acceleration in solar flares. The presence of an inhomogeneous, extended acceleration region produces a spectral index that is, in most cases, different from the simple leaky-box prediction. In particular, it results in a generally softer spectral index than predicted by the leaky-box solution, for both scatter-free and diffusive transport, and thus should be taken into account when modelling stochastic acceleration in solar flares." @default.
• W3098895887 created "2020-11-23" @default.
• W3098895887 creator A5029418190 @default.
• W3098895887 creator A5054079921 @default.
• W3098895887 date "2018-04-01" @default.
• W3098895887 modified "2023-09-26" @default.
• W3098895887 title "Spatially inhomogeneous acceleration of electrons in solar flares" @default.
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• W3098895887 doi "https://doi.org/10.1051/0004-6361/201730708" @default.
• W3098895887 hasPublicationYear "2018" @default.
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