Collisionless turbulent transport and anisotropic electron heating in coronal flare loops
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201117186/pdf
Reference37 articles.
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2. Deconvolution of Directly Precipitating and Trap‐Precipitating Electrons in Solar Flare Hard X‐Rays. I. Method and Tests
3. Aschwanden, M. J. 1998b, in Observational Plasma Astrophysics: Five Years of YOHKOH and Beyond, ed. T. Watanabe et al., Astrophys. Space Sci. Lib. (Boston, Mass.: Kluwer Academic Publishers), 229, 285
4. Accuracy, Uncertainties, and Delay Distribution of Electron Time-of-Flight Measurements in Solar Flares
5. The Inversion of Electron Time-of-Flight Distances from Hard X-Ray Time Delay Measurements
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3. Non-Maxwellian electron distribution functions due to self-generated turbulence in collisionless guide-field reconnection;Physics of Plasmas;2016-10
4. SUPPRESSION OF ENERGETIC ELECTRON TRANSPORT IN FLARES BY DOUBLE LAYERS;The Astrophysical Journal;2012-08-31
5. Observational Aspects of Particle Acceleration in Large Solar Flares;Space Science Reviews;2012-06-12
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