Hysteresis of indices of solar and ionospheric activity during 11-year cycles
- Авторлар: Bruevich E.A.1, Kazachevskaya T.V.2, Katyushina V.V.2, Nusinov A.A.2, Yakunina G.V.1
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Мекемелер:
- Sternberg Astronomical Institute
- Federov Institute of Applied Geophysics
- Шығарылым: Том 56, № 8 (2016)
- Беттер: 1075-1081
- Бөлім: Article
- URL: https://journal-vniispk.ru/0016-7932/article/view/156042
- DOI: https://doi.org/10.1134/S001679321608003X
- ID: 156042
Дәйексөз келтіру
Аннотация
The effects of hysteresis, which is a manifestation of ambiguous relationships between different solar activity indices during the rising and declining phases of solar cycles, are analyzed. The paper addresses the indices characterizing radiation from the solar photosphere, chromosphere, and corona, and the ionospheric indices. The 21st, 22nd, and 23rd solar cycles, which significantly differ from each other in amplitude, exhibit different extents of hysteresis.
Авторлар туралы
E. Bruevich
Sternberg Astronomical Institute
Хат алмасуға жауапты Автор.
Email: red-field@yandex.ru
Ресей, Moscow, 119991
T. Kazachevskaya
Federov Institute of Applied Geophysics
Email: red-field@yandex.ru
Ресей, Moscow, 129128
V. Katyushina
Federov Institute of Applied Geophysics
Email: red-field@yandex.ru
Ресей, Moscow, 129128
A. Nusinov
Federov Institute of Applied Geophysics
Email: red-field@yandex.ru
Ресей, Moscow, 129128
G. Yakunina
Sternberg Astronomical Institute
Email: red-field@yandex.ru
Ресей, Moscow, 119991
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