Relationship of the stable auroral red arcs height to solar activity. The observation results at the Yakutsk meridian

I. B. Ievenko; Иевенко И. Б.; S. G. Parnikov; Парников С. Г.; A. V. Sokolnikov; Сокольников А. В.

doi:10.31857/S0367676522700454

Relationship of the stable auroral red arcs height to solar activity. The observation results at the Yakutsk meridian

Авторлар: Ievenko I.¹, Parnikov S.¹, Sokolnikov A.¹
Мекемелер:
1. Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
Шығарылым: Том 87, № 2 (2023)
Беттер: 254-261
Бөлім: Articles
URL: https://journals.rcsi.science/0367-6765/article/view/135281
DOI: https://doi.org/10.31857/S0367676522700454
EDN: https://elibrary.ru/AIMSUY
ID: 135281

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Аннотация
Авторлар туралы
Әдебиет тізімі
Қосымша файлдар
Статистика

Аннотация

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.

Авторлар туралы

I. Ievenko

Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch
of the Russian Academy of Sciences

Хат алмасуға жауапты Автор.
Email: ievenko@ikfia.ysn.ru
Russia, 677027, Yakutsk

S. Parnikov

Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch
of 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 Branch
of the Russian Academy of Sciences

Email: ievenko@ikfia.ysn.ru
Russia, 677027, Yakutsk

Әдебиет тізімі

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