Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm

Данилова Ольга Александровна; Птицына Наталья Григорьевна; Сдобнов Валерий Евгеньевич

doi:10.12737/stp-103202408

УДК 52

HYSTERESIS PHENOMENA IN THE RESPONSE OF GEOMAGNETIC ACTIVITY AND COSMIC RAY PARAMETERS TO VARIATIONS IN THE INTERPLANETARY MEDIUM DURING A MAGNETIC STORM Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm

АА Аа

Опубликовано в Solar-Terrestrial Physics · Том 10, Номер 3 · Страницы 66–74 · Рубрика: 19TH ANNUAL CONFERENCE “PLASMA PHYSICS IN THE SOLAR SYSTEM”. FEBRUARY 5–9, 2024, SPACE RESEARCH INSTITUTE RAS, MOSCOW, RUSSIA

DOI: https://doi.org/10.12737/stp-103202408

Получено: 30.03.2024 Одобрено: 21.05.2024 Опубликовано: 29.09.2024 Язык публикаций: ENG

Авторы

ДА

Данилова Ольга Александровна

ПТ

Птицына Наталья Григорьевна

СД

Сдобнов Валерий Евгеньевич

ДА

Данилова Ольга Александровна

Ученая степень: кандидат физико-математических наук

Санкт-Петербургский филиал Института земного магнетизма, ионосферы и распространения радиоволн им. Н.В. Пушкова РАН Россия · Санкт-Петербург

ПТ

Птицына Наталья Григорьевна

Ученая степень: кандидат физико-математических наук

Санкт-Петербургский филиал Института земного магнетизма, ионосферы и распространения радиоволн РАН Россия · Санкт-Петербург

СД

Сдобнов Валерий Евгеньевич

Ученая степень: доктор физико-математических наук

Институт солнечно-земной физики СО РАН Россия · Иркутск

АННОТАЦИЯ

The dynamics of the intensity of cosmic rays is known to be different on the ascending and descending branches of the 11-year solar cycle, i.e., hysteresis phenomena are observed. Recently, it has been obtained that at shorter intervals on the scale of magnetic storms there are also signs of hysteresis in dependences of cosmic ray cutoff rigidities R (geomagnetic thresholds) on heliosphere and geosphere parameters. R is the rigidity below which a particle flux is cut off due to geomagnetic shielding. In this paper, we have analyzed the dependence of the geomagnetic storm index Dst and the variation of the ΔR thresholds on interplanetary magnetic field (IMF) and solar wind (SW) parameters during the two-step magnetic storm on September 7–8, 2017. We have found hysteresis phenomena in the following paired series: (1) dependences of Dst on SW and IMF parameters, and (2) dependences of ΔR on SW and IMF parameters. We have established that the dependence curves in the storm descending phase (main phase) and ascending phase (recovery phase) do not coincide — hysteresis loops are formed. A specific feature of the storm under study is the second lowering of Dst in the recovery phase. The hysteresis pattern reflects this specific storm dynamics, forming two hysteresis loops in response to the two Dst drops.

КЛЮЧЕВЫЕ СЛОВА

cosmic rays, geomagnetic threshold, cosmic ray cutoff rigidities, supersubstorm, interplanetary magnetic field, geomagnetic activity

Финансирование

The work was partially carried out with the financial support from the Ministry of Science and Higher Education of the Russian Federation (Subsidy No. 075-GZ/Ts3569/278)

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Жеребцов Гелий Александрович

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ГОСТ

Данилова О. А., Птицына Н. Г., Сдобнов В. Е. Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm // Solar-Terrestrial Physics. 2024. №. 3. С. 66-74. DOI: https://doi.org/10.12737/stp-103202408. (дата обращения: 22.09.2026).

MLA

Данилова Ольга Александровна, Птицына Н. Г., Сдобнов В. Е.. "Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm." Solar-Terrestrial Physics 10.3 (2024): 66-74. DOI: https://doi.org/10.12737/stp-103202408.

APA

Данилова О. А., Птицына Н. Г., Сдобнов В. Е. (2024). Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm. Solar-Terrestrial Physics, 10(3), 66-74. https://doi.org/10.12737/stp-103202408

Chicago

Данилова Ольга Александровна, Птицына Н. Г., Сдобнов В. Е.. "Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm." Solar-Terrestrial Physics 10, no. 3 (2024): 66-74. https://doi.org/10.12737/stp-103202408.

WIKI

{{cite journal | author = Данилова О. А., Птицына Н. Г., Сдобнов В. Е. | title = Hysteresis phenomena in the response of geomagnetic activity and cosmic ray parameters to variations in the interplanetary medium during a magnetic storm | journal = Solar-Terrestrial Physics | year = 2024 | volume = 10 | issue = 3 | pages = 66-74 | doi = 10.12737/stp-103202408 }}

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