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pro vyhledávání: '"Somov, Boris V"'
Autor:
Dumin, Yurii V., Somov, Boris V.
Solar flares - which are the most prominent manifestation of the solar activity - typically manifest themselves as a single or a set of luminous arcs (magnetic flux tubes) rooted in regions of opposite polarity in the photosphere. However, a careful
Externí odkaz:
http://arxiv.org/abs/2309.16417
Publikováno v:
Physica D 436 (2022) 133320
The so-called "anemone" solar flares are an interesting type of the space plasma phenomena, where multiple null points of the magnetic field are connected with each other and with the magnetic sources by the separators, thereby producing the complex
Externí odkaz:
http://arxiv.org/abs/2111.06730
Autor:
Dumin, Yurii V., Somov, Boris V.
The chromospheric anemone microflares (AMF) are the transient solar phenomena whose emission regions have a multi-ribbon configuration. As distinct from the so-called "atypical" solar flares, also possessing a few ribbons, the temporal and spatial sc
Externí odkaz:
http://arxiv.org/abs/1904.09439
Publikováno v:
In Physica D: Nonlinear Phenomena August 2022 436
Autor:
Dumin, Yurii V., Somov, Boris V.
Publikováno v:
Research Notes of the American Astronomical Society, Vol. 1, No. 1, Article Id. 15 (2017)
We report on observation of the unusual kind of solar microflares, presumably associated with the so-called "topological trigger" of magnetic reconnection, which was theoretically suggested long time ago by Gorbachev et al. (Sov. Ast. 1988, v.32, p.3
Externí odkaz:
http://arxiv.org/abs/1711.03140
Autor:
Dumin, Yurii V., Somov, Boris V.
The probability of occurrence of various topological configurations of the 3D null-point reconnection in a random magnetic field is studied. It is found that the non-axisymmetrical six-tail configuration (or "improper radial null") should play the do
Externí odkaz:
http://arxiv.org/abs/1407.6039
Autor:
Somov, Boris V.
Publikováno v:
Asian Journal of Physics, Vol. 17, Nos. 2-3, 421-454, 2008
Solar 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
Externí odkaz:
http://arxiv.org/abs/0901.4697
Autor:
Dumin, Yurii V, Somov, Boris V
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters; Feb2024, Vol. 528 Issue 1, pL15-L19, 5p
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