Enviar artigo por via de e-mail Relationship of the stable auroral red arcs height to solar activity. The observation results at the Yakutsk meridian
- Autores: Ievenko I.B.1, Parnikov S.G.1, Sokolnikov A.V.1
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Afiliações:
- Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
- Edição: Volume 87, Nº 2 (2023)
- Páginas: 254-261
- Seção: Articles
- URL: https://rjeid.com/0367-6765/article/view/654486
- DOI: https://doi.org/10.31857/S0367676522700454
- EDN: https://elibrary.ru/AIMSUY
- ID: 654486
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Resumo
We presented the first results of triangulation measurements of the stable auroral red arcs height at the Yakutsk meridian in 2015–2020. The heights of the lower luminosity boundary in arcs of 350–370 km near the maximum and 250–290 km during the minimum of solar activity in the 24th cycle are obtained. The decrease of the red arcs height in the minimum years is due to the significant density decrease of the upper neutral atmosphere.
Sobre autores
I. Ievenko
Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branchof the Russian Academy of Sciences
Autor responsável pela correspondência
Email: ievenko@ikfia.ysn.ru
Russia, 677027, Yakutsk
S. Parnikov
Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branchof the Russian Academy of Sciences
Email: ievenko@ikfia.ysn.ru
Russia, 677027, Yakutsk
A. Sokolnikov
Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branchof the Russian Academy of Sciences
Email: ievenko@ikfia.ysn.ru
Russia, 677027, Yakutsk
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