MANIFESTATION OF SOLAR ACTIVITY AND DYNAMICS OF THE ATMOSPHERE IN VARIATIONS OF 577.7 AND 630.0 nm ATMOSPHERIC EMISSIONS IN SOLAR CYCLE 24

In the paper, variations of the night emission intensities in the 557.7 and 630 nm atomic oxygen lines [OI] in 2011–2019 have been analyzed. The analysis is based on data from the ISTP SB RAS Geophysical Observatory. The emission intensities are compared with atmospheric, solar, and geophysical para...

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Bibliographic Details
Main Author: A.V. Mikhalev
Format: Article
Language:English
Published: INFRA-M 2020-09-01
Series:Solar-Terrestrial Physics
Subjects:
Online Access:https://naukaru.ru/en/nauka/article/39470/view