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

作者: Ievenko I.¹, Parnikov S.¹, Sokolnikov A.¹
隶属关系:
1. Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
期: 卷 87, 编号 2 (2023)
页面: 254-261
栏目: 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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详细

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.

作者简介

I. Ievenko

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

编辑信件的主要联系方式.
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

参考

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