Coronal current sheet as a source of thermal X-rays
Author:
Publisher
Pleiades Publishing Ltd
Subject
Space and Planetary Science,Geophysics
Link
http://link.springer.com/content/pdf/10.1134/S001679321407010X.pdf
Reference8 articles.
1. Lin, R.P., Krucker, S., Hurford, G.J., et al., RHESSI observations of particles acceleration and energy release in an intense gamma-ray line flare, Astrophys. J., 2003, vol. 595, no. 2, p. L69.
2. Masuda, S., Kosugi, T., Hara, H., Tsuneta, S., and Ogawara, Y., A loop-top hard X-ray source in a compact solar flare as evidence for magnetic reconnection, Nature, 1994, vol. 371, no. 6497, pp. 495–497.
3. Podgorny, A.I., The magnetohydrodynamical instability of a current sheet created by plasma flow, Plasma Phys. Control. Fusion, 1989, vol. 31, no. 8, pp. 1271–1279.
4. Podgorny, A.I. and Podgorny, I.M., A model of solar flare: Comparisons with observations of high-energy processes, Astron. Rep., 2006, vol. 50, no. 10, pp. 842–850.
5. Podgorny, A.I. and Podgorny, I.M., Formation of several current sheets preceding a series of flares above the active region AR 10365, Astron. Rep., 2008, vol. 52, no. 8, pp. 666–675.
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