Abstract
The relationship between the production of γ-ray emitting particles and non-thermal soft X-ray line broadening is investigated. A model of particle acceleration via the stochastic interaction with MHD turbulence is assumed and the time development of the wave energy density derived under the condition of energy conservation between waves and particles. The inferred numbers and energy distribution of accelerated protons for four γ-ray flares are used to define the wave energy density and its temporal development. The presence of Alfvén wave turbulence is considered as the source of the non-thermal motions in the ambient plasma. These motions are observed as excess widths in the soft X-ray line emission from these events. The decay of the waves via the particle acceleration process is compared with the observed decays of this non-thermal line broadening. Our results show that both the γ-ray emission and excess soft X-ray line widths in these flares can be explained by the single physical phenomenon of Alfvén wave turbulence.
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Alexander, D., Matthews, S.A. Particle acceleration and the decay of soft X-ray non-thermal line broadening in solar flares. Sol Phys 154, 157–175 (1994). https://doi.org/10.1007/BF00676781
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DOI: https://doi.org/10.1007/BF00676781