Мақаланы E-mail арқылы жіберу Analysis of Oscillatory Modes of the Magnetic Field of Solar Facular Formations
- Авторлар: Strekalova P.V.1, Nagovitsyn Y.A.1,2, Smirnova V.V.1
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Мекемелер:
- Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
- St. Petersburg State University of Aerospace Instrumentation
- Шығарылым: Том 58, № 7 (2018)
- Беттер: 893-898
- Бөлім: Article
- URL: https://journal-vniispk.ru/0016-7932/article/view/157024
- DOI: https://doi.org/10.1134/S0016793218070204
- ID: 157024
Дәйексөз келтіру
Ашық рұқсат
Рұқсат берілді
Тек жазылушылар үшін
Аннотация
Quasi-periodical variations in the magnetic fields of long-living, small-scale magnetic structures, solar facular formations (FFs), are analyzed. We used the method of Empirical Mode Decomposition (EMD) to reveal the empirical modes of time series of magnetic field variations in four FFs and tested them for the existence of coloured noise. We proposed a qualitative interpretation of statistically reliable oscillatory modes.
Авторлар туралы
P. Strekalova
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
Хат алмасуға жауапты Автор.
Email: auriga-lynx@yandex.ru
Ресей, St. Petersburg
Yu. Nagovitsyn
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences; St. Petersburg State University of Aerospace Instrumentation
Email: auriga-lynx@yandex.ru
Ресей, St. Petersburg; St. Petersburg
V. Smirnova
Central Astronomical Observatory at Pulkovo of the Russian Academy of Sciences
Email: auriga-lynx@yandex.ru
Ресей, St. Petersburg
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