- PII
- S30345170S0004629925010068-1
- DOI
- 10.7868/S3034517025010068
- Publication type
- Article
- Status
- Published
- Authors
- Volume/ Edition
- Volume 102 / Issue number 1
- Pages
- 66-70
- Abstract
- 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.
- Keywords
- Солнце вспышки ускорение частиц
- Date of publication
- 22.01.2026
- Year of publication
- 2026
- Number of purchasers
- 0
- Views
- 47
References
- 1. J. Threlfall, T. Neukirch, C.E. Parnell, O.S. Eradat, Astron. and Astrophys. 574, A7, 15 (2015).
- 2. A.V. Getling, R. Ishikawa, A.A. Buchnev, Advances in Space Research 55, 862 (2015).
- 3. М.М. Молоденский, В.Л. Мерзляков, Письма в Астрон. журн. 28, 314 (2002).
- 4. А.С. Кириченко, С.А. Богачев, Письма в Астрон. журн. 39, 884 (2013).
- 5. A. Warmuth, G. Mann, Astron. and Astrophys. 588, A115, 14 (2016).
- 6. В.Л. Мерзляков, Доклад на Всероссийской конференции “Магнетизм и активность Солнца — 2022” (КрАО РАН, Крым, 22-26 августа, 2022).
