Magnetic reconnection and topological trigger in physics of large solar flares

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dc.creatorSomov, Boris V.
dc.date2009-01-29
dc.date.accessioned2026-07-07T12:35:37Z
dc.date.available2026-07-07T12:35:37Z
dc.descriptionSolar flares are accessible to a broad variety of observational methods to see and investigate the {\em magnetic reconnection} phenomenon in high-temperature strongly-magnetized plasma of the solar corona. An analysis of the topological peculiarities of magnetic field in active regions shows that the {\em topological trigger} effect is necessary to allow for in order to construct models for large eruptive flares. The topological trigger is not a resistive instability which leads to a change of the topology of the field configuration from pre- to post reconnection state. On the contrary, the topological trigger is a quick change of the global topology, which dictates the fast reconnection of collisional or collisionless nature. The current state of the art and development potential of the theory of collisionless reconnection in the strong magnetic fields related to large flares are briefly reviewed. Particle acceleration is considered in collapsing magnetic traps created by reconnection. In order to explain the formation of coronal X-ray sources, the Fermi acceleration and betatron mechanism are simultaneously taken into account analytically in a collisionless approximation. Finally, the emphasis is on urgent unsolved problems of solar flare physics.
dc.description38 pages, 20 figures
dc.identifierhttps://arxiv.org/abs/0901.4697
dc.identifierhttp://arxiv.org/abs/0901.4697
dc.identifierAsian Journal of Physics, Vol. 17, Nos. 2-3, 421-454, 2008
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/217823
dc.subjectSolar and Stellar Astrophysics
dc.subjectHigh Energy Astrophysical Phenomena
dc.titleMagnetic reconnection and topological trigger in physics of large solar flares
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