Solar flare phenomena forecast: solar proton events
- Авторлар: Ishkov V.1
-
Мекемелер:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Science
- Шығарылым: Том 87, № 7 (2023)
- Беттер: 1010-1013
- Бөлім: Articles
- URL: https://journals.rcsi.science/0367-6765/article/view/135438
- DOI: https://doi.org/10.31857/S0367676523701788
- EDN: https://elibrary.ru/OSEKDF
- ID: 135438
Дәйексөз келтіру
Аннотация
The problems of predicting solar flare events, the only source of high-energy protons, both from the process of energy release itself and from the accompanying dynamic phenomena: shock waves and coronal mass ejections propagating from the place of energy release, are considered from modern positions. The possibility of predicting the flare events themselves ensures the interaction of new emerging magnetic fluxes with the magnetic fields of active regions and outside them, but always on the dividing line of polarities. The possibility of the release of solar protons during of a flare event is determined by the characteristics and localization of the flare event, its CME parameters, and the ratio of its energy in different radiation ranges.
Авторлар туралы
V. Ishkov
Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Science
Хат алмасуға жауапты Автор.
Email: ishkov@izmiran.ru
Russia, 108840, Moscow
Әдебиет тізімі
- Ишков В.Н. // Изв. РАН. Сер. физ. 1998. Т. 62. № 9. С. 1835.
- Ишков В.Н. // Изв. РАН. Сер. физ. 1999. Т. 63. № 11. С. 2148.
- де Ягер К. // Строение и динамика атмосферы Солнца. Москва: Изд. иностр. лит., 1962. 376 с.
- Головко А.А. // Солн. данные. 1986. № 4. С. 48.
- Kahler S.W., Cliver E.W., Ling A.G. // JASTP. 2007. V. 69. No. 1-2. P. 43.
- Balch C. // Space Weather. 2008. V. 6. Art. No. S01001.
- Belov A. // Adv. Space Res. 2009. V. 43. No. 4. P. 467.
- Posner A. // Space Weather. 2007. V. 5. Art. No. S05001.
- Núñez M. // Space Weather. 2011. V. 9. Art. No. S07003.
- Núñez M. // Space Weather. 2015. V. 13. P. 807.