Modeling of Physical Processes by Analysis of Hard X-Ray and Microwave Radiations in the Solar Flare of November 10, 2002
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Geophysics
Link
http://link.springer.com/article/10.1134/S0016793217080060/fulltext.html
Reference21 articles.
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3. Bykov, A.M. and Fleishman, G.D., Particle acceleration by strong turbulence in solar flares: Theory of spectrum evolution, Astrophys. J., 2009, vol. 692, no. 1, pp. L45–L49.
4. Charikov, Y.E., Melnikov, V.F., and Kudryavtsev, I.V., Intensity and polarization of the hard X-ray radiation of solar flares at the top and footpoints of a magnetic loop, Geomagn. Aeron. (Engl. Transl.), 2012, vol. 52, no. 8, pp. 1021–1031.
5. Charikov, Y.E. and Shabalin, A.N., Hard X-ray generation in the turbulent plasma of solar flares, Geomagn. Aeron. (Engl. Transl.), 2016, vol. 56, no. 8, pp. 1068–1074.
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