Enviar artigo por via de e-mail THE DIFFERENT FACTORS INFLUENCE ON THE SOLAR FLARES ENERGY
- Autores: Merzlyakov V.L1
-
Afiliações:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation
- Edição: Volume 102, Nº 1 (2025)
- Páginas: 66-70
- Seção: Articles
- URL: https://medbiosci.ru/0004-6299/article/view/289090
- DOI: https://doi.org/10.31857/S0004629925010068
- EDN: https://elibrary.ru/HLSRMW
- ID: 289090
Citar
Texto integral
Resumo
The factors influencing the energy of the solar flare are being studied. The model of particle acceleration in the magnetic X-singularity is investigated. It was found that the flare energy depends mainly on the flow of electrons into the acceleration zone. The change in such a flow is determined by the size of the acceleration zone. It is calculated that for a chromospheric flare source the vertical length of the acceleration zone varies from ∼100 km to ≈ 2 ⋅ 103 km and its diameter varies from ∼1 km to ≈ 100 km.
Palavras-chave
Sobre autores
V. Merzlyakov
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation
Email: mvl@izmiran.ru
Troitsk, Russia
Bibliografia
- J. Threlfall, T. Neukirch, C.E. Parnell, O.S. Eradat, Astron. and Astrophys. 574, A7, 15 (2015).
- A.V. Getling, R. Ishikawa, A.A. Buchnev, Advances in Space Research 55, 862 (2015).
- М.М. Молоденский, В.Л. Мерзляков, Письма в Астрон. журн. 28, 314 (2002).
- А.С. Кириченко, С.А. Богачев, Письма в Астрон. журн. 39, 884 (2013).
- A. Warmuth, G. Mann, Astron. and Astrophys. 588, A115, 14 (2016).
- В.Л. Мерзляков, Доклад на Всероссийской конференции “Магнетизм и активность Солнца — 2022” (КрАО РАН, Крым, 22-26 августа, 2022).
Arquivos suplementares
