Topside ionosphere during solar cosmic ray bursts and Forbush decreases in galactic cosmic rays

Valery Yanchukovsky; Anastasiya Belinskaya

doi:10.12737/stp-83202205

UDC 55

TOPSIDE IONOSPHERE DURING SOLAR COSMIC RAY BURSTS AND FORBUSH DECREASES IN GALACTIC COSMIC RAYS Topside ionosphere during solar cosmic ray bursts and Forbush decreases in galactic cosmic rays

АА Аа

Published in Solar-Terrestrial Physics · Volume 8, Issue 3 · Pages 32–37 · Rubric: Results of current research

DOI: https://doi.org/10.12737/stp-83202205

Received: 18.05.2022 Accepted: 03.08.2022 Published: 30.09.2022 Language of publication: ENG

Authors

Valery Yanchukovsky

Anastasiya Belinskaya

ORCID

Valery Yanchukovsky

Academic degree: doctor of physical and mathematical sciences

Trofimuk Institute of Petroleum Geology and Geophysics SB RAS Russian Federation · Novosibirsk

Anastasiya Belinskaya

Academic degree: candidate of physical and mathematical sciences

Trofimuk Institute of Petroleum Geology and Geophysics SB RAS Russian Federation · Novosibirsk

ORCID

ABSTRACT

The paper considers the behavior of the upper ionosphere at heights of the F2 layer during Forbush decreases in galactic cosmic rays (GCR FDs) and solar cosmic ray (SCR) bursts. We use the results of long-term continuous observations of cosmic rays and the ionosphere in Novosibirsk for the period from 1968 to 2021. The ionospheric disturbances in the F2 layer during GCR FDs, which were accompanied by a magnetic storm, took the form of an ionospheric storm negative phase. The scale of the negative phase of the ionospheric F-layer disturbance increases with increasing Dst index of the geomagnetic storm. This increase in the amplitude of the ionospheric disturbance becomes more and more significant depending on the magnitude of Forbush decreases. A burst of the amplitude of the daily variation in the F2-layer critical frequency occurred eight days after SCR bursts and GCR FD front. We assume that this burst might have been caused by disturbances in the lower atmosphere due to significant variations in the intensity of SCR and GCR fluxes.

KEYWORDS

solar cosmic rays, galactic cosmic rays, ionosphere, geomagnetic disturbance

Funding

The work was financially supported by the Ministry of Science and Higher Education of the Russian Federation (Project FWZZ-2022-0019)

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Geliy Zherebtsov

solater@iszf.irk.ru

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stepanov@gaoran.ru

Deputy Editor-in-Chief

Alexander Potapov

potapov@iszf.irk.ru

Executive Secretary of Editorial Board

Natalia Polyushkina

npol@iszf.irk.ru

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GOST

Yanchukovsky V. L., Belinskaya A. Y. Topside ionosphere during solar cosmic ray bursts and Forbush decreases in galactic cosmic rays // Solar-Terrestrial Physics. 2022. no. 3. pp. 32-37. DOI: https://doi.org/10.12737/stp-83202205. (Date of access 13.10.2026).

MLA

Valery Yanchukovsky, Belinskaya A. Y.. "Topside ionosphere during solar cosmic ray bursts and Forbush decreases in galactic cosmic rays." Solar-Terrestrial Physics 8.3 (2022): 32-37. DOI: https://doi.org/10.12737/stp-83202205.

APA

Yanchukovsky V. L., Belinskaya A. Y. (2022). Topside ionosphere during solar cosmic ray bursts and Forbush decreases in galactic cosmic rays. Solar-Terrestrial Physics, 8(3), 32-37. https://doi.org/10.12737/stp-83202205

Chicago

Valery Yanchukovsky, Belinskaya A. Y.. "Topside ionosphere during solar cosmic ray bursts and Forbush decreases in galactic cosmic rays." Solar-Terrestrial Physics 8, no. 3 (2022): 32-37. https://doi.org/10.12737/stp-83202205.

WIKI

{{cite journal | author = Yanchukovsky V. L., Belinskaya A. Y. | title = Topside ionosphere during solar cosmic ray bursts and Forbush decreases in galactic cosmic rays | journal = Solar-Terrestrial Physics | year = 2022 | volume = 8 | issue = 3 | pages = 32-37 | doi = 10.12737/stp-83202205 }}

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TOPSIDE IONOSPHERE DURING SOLAR COSMIC RAY BURSTS AND FORBUSH DECREASES IN GALACTIC COSMIC RAYS Topside ionosphere during solar cosmic ray bursts and Forbush decreases in galactic cosmic rays

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