Magnetic Reconnections And the Bastille Day
- Autores: Ledentsov L.S1, Somov B.V1
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Afiliações:
- Sternberg Astronomical Institute, Lomonosov Moscow State University
- Edição: Nº 4 (2021)
- Páginas: 8-23
- Seção: Articles
- URL: https://journals.eco-vector.com/0044-3948/article/view/630959
- DOI: https://doi.org/10.7868/S0044394821040010
- ID: 630959
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Resumo
In modern astrophysics — particularly, in X-ray and gamma-ray astronomy — solar flares have become a kind of standard in the studies of flare processes of electromagnetic nature. In contrast to the analogous phenomena in other stars the solar flares provide an opportunity for the comprehensive study of magnetic reconnections in both the high-temperature highly magnetised plasma of the Sun's corona and low-temperature weakly ionised plasma of the photosphere.
Sobre autores
L. Ledentsov
Sternberg Astronomical Institute, Lomonosov Moscow State UniversityMoscow, Russia
B. Somov
Sternberg Astronomical Institute, Lomonosov Moscow State UniversityMoscow, Russia
Bibliografia
- Somov B.V. Plasma Astrophysics, Part I, Fundamental and Practice, Second Edition. New York: Springer, 2013.
- Somov B.V. Plasma Astrophysics, Part II, Reconnection and Flares, Second Edition. New York: Springer, 2012.
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