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Title: Onset of electron acceleration in a flare loop

Abstract

We carried out a detailed analysis of X-ray and radio observations of a simple flare loop that occurred on 2002 August 12, with the impulsive hard X-ray (HXR) light curves dominated by a single pulse. The emission spectra of the early impulsive phase are consistent with an isothermal model in the coronal loop with a temperature reaching several keV. A power-law high-energy spectral tail is evident near the HXR peak time, in accordance with the appearance of footpoints at high energies, and is well correlated with the radio emission. The energy content of the thermal component keeps increasing gradually after the disappearance of this nonthermal component. These results suggest that electron acceleration only covers the central period of a longer and more gradual energy dissipation process and that the electron transport within the loop plays a crucial role in the formation of the inferred power-law electron distribution. The spectral index of power-law photons shows a very gradual evolution, indicating that the electron accelerator is in a quasi-steady state, which is confirmed by radio observations. These results are consistent with the theory of stochastic electron acceleration from a thermal background. Advanced modeling with coupled electron acceleration and spatial transport processes ismore » needed to explain these observations more quantitatively, which may reveal the dependence of the electron acceleration on the spatial structure of the acceleration region.« less

Authors:
;  [1];  [2]
  1. Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210008 (China)
  2. School of Physics and Astronomy, SUPA, University of Glasgow, Glasgow, G12 8QQ (United Kingdom)
Publication Date:
OSTI Identifier:
22365026
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal
Additional Journal Information:
Journal Volume: 793; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0004-637X
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; COSMIC RADIO SOURCES; COSMIC X-RAY SOURCES; DISTRIBUTION; ELECTRONS; EMISSION; EMISSION SPECTRA; GAMMA RADIATION; GRAY ENERGY; HARD X RADIATION; KEV RANGE; PHOTONS; PLASMA; SIMULATION; STAR EVOLUTION; STEADY-STATE CONDITIONS; STOCHASTIC PROCESSES; SUN; TURBULENCE; VISIBLE RADIATION

Citation Formats

Sharykin, Ivan, Liu, Siming, and Fletcher, Lyndsay, E-mail: liusm@pmo.ac.cn. Onset of electron acceleration in a flare loop. United States: N. p., 2014. Web. doi:10.1088/0004-637X/793/1/25.
Sharykin, Ivan, Liu, Siming, & Fletcher, Lyndsay, E-mail: liusm@pmo.ac.cn. Onset of electron acceleration in a flare loop. United States. doi:10.1088/0004-637X/793/1/25.
Sharykin, Ivan, Liu, Siming, and Fletcher, Lyndsay, E-mail: liusm@pmo.ac.cn. Sat . "Onset of electron acceleration in a flare loop". United States. doi:10.1088/0004-637X/793/1/25.
@article{osti_22365026,
title = {Onset of electron acceleration in a flare loop},
author = {Sharykin, Ivan and Liu, Siming and Fletcher, Lyndsay, E-mail: liusm@pmo.ac.cn},
abstractNote = {We carried out a detailed analysis of X-ray and radio observations of a simple flare loop that occurred on 2002 August 12, with the impulsive hard X-ray (HXR) light curves dominated by a single pulse. The emission spectra of the early impulsive phase are consistent with an isothermal model in the coronal loop with a temperature reaching several keV. A power-law high-energy spectral tail is evident near the HXR peak time, in accordance with the appearance of footpoints at high energies, and is well correlated with the radio emission. The energy content of the thermal component keeps increasing gradually after the disappearance of this nonthermal component. These results suggest that electron acceleration only covers the central period of a longer and more gradual energy dissipation process and that the electron transport within the loop plays a crucial role in the formation of the inferred power-law electron distribution. The spectral index of power-law photons shows a very gradual evolution, indicating that the electron accelerator is in a quasi-steady state, which is confirmed by radio observations. These results are consistent with the theory of stochastic electron acceleration from a thermal background. Advanced modeling with coupled electron acceleration and spatial transport processes is needed to explain these observations more quantitatively, which may reveal the dependence of the electron acceleration on the spatial structure of the acceleration region.},
doi = {10.1088/0004-637X/793/1/25},
journal = {Astrophysical Journal},
issn = {0004-637X},
number = 1,
volume = 793,
place = {United States},
year = {2014},
month = {9}
}