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Impulsive Flare Plasma Energization in the Light of Yohkoh Discoveries

Published online by Cambridge University Press:  25 May 2016

Yurii M. Voitenko*
Affiliation:
Department of Space Plasma Physics, Main Astronomical Observatory, Holosiiv, Kyiv-22, 252650, Ukraine

Extract

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Flare scenario, based on Yohkoh observations and magnetic reconnection (MR) hypotesis, has been elaborated recently (Tsuneta, 1996; Shibata, 1997). Using theoretical prediction that the fast MR results in a high-speed outflows from reconnection site, the reconnection downflow has been supposed to collide with the top of underlying magnetic loop, producing superhot plasma and high-energy particles.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Copyright
Copyright © Kluwer 1998 

References

Masuda, S., Kosugi, T., Hara, H., Sakao, T., Shibata, K., and Tsuneta, S.: 1995, P.A.S.J. 47, 677 Google Scholar
Shibata, K.: 1997, in Watanabe, T., Kosugi, T., and Sterling, A. C. (eds) Proc. Yohkoh 5th Anniversary Symposium , in press.Google Scholar
Simnett, G. M.: 1995, Space Sci. Rev. 73, 387.Google Scholar
Strachan, N. R. and Priest, E. R.: 1994, Geophys. Astrophys. Fluid Dynamics 74, 245274 Google Scholar
Tsuneta, S.: 1996, Astrophys. J. 456, 840.Google Scholar
Voitenko, Yu. M.: 1996a, Solar Phys. 168, 219.CrossRefGoogle Scholar
Voitenko, Yu. M.: 1996b, ASP Conference Series 111, 312.Google Scholar