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

Authors: Ievenko I.B.¹, Parnikov S.G.¹, Sokolnikov A.V.¹
Affiliations:
1. Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
Issue: Vol 87, No 2 (2023)
Pages: 254-261
Section: Articles
URL: https://ruspoj.com/0367-6765/article/view/654486
DOI: https://doi.org/10.31857/S0367676522700454
EDN: https://elibrary.ru/AIMSUY
ID: 654486

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Abstract

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.

About the authors

I. B. Ievenko

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

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

S. G. 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. V. 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

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