Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure

Пархомов Владимир Александрович; Еселевич Виктор Григорьевич; Еселевич Максим Викторович; Дмитриев Алексей Владимирович; Суворова Алла Васильевна; Хомутов Сергей Юрьевич; Цэгмэд Баттуулай; Теро Райта

doi:10.12737/stp-73202102

УДК 52 УДК 53

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MAGNETOSPHERIC RESPONSE TO THE INTERACTION WITH THE SPORADIC SOLAR WIND DIAMAGNETIC STRUCTURE Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure

АА Аа

Опубликовано в Solar-Terrestrial Physics · Том 7, Номер 3 · Страницы 11–28 · Рубрика: Results of current research

DOI: https://doi.org/10.12737/stp-73202102

Получено: 27.01.2021 Одобрено: 28.06.2021 Язык публикаций: ENG

Авторы

ПА

Пархомов Владимир Александрович

ЕС

Еселевич Виктор Григорьевич

ЕС

Еселевич Максим Викторович

ДМ

Дмитриев Алексей Владимирович

и др.

СУ

Суворова Алла Васильевна

ХО

Хомутов Сергей Юрьевич

ЦЭ

Цэгмэд Баттуулай

ТЕ

Теро Райта

ПА

Пархомов Владимир Александрович

Ученая степень: доктор физико-математических наук

Байкальский государственный университет профессор защита информации · кафедра математических методов и цифровых технологий · Россия · Иркутск

ЕС

Еселевич Виктор Григорьевич

Ученая степень: доктор физико-математических наук

Институт солнечно-земной физики СО РАН Россия · Иркутск

ЕС

Еселевич Максим Викторович

Ученая степень: кандидат физико-математических наук

Институт солнечно-земной физики СО РАН Россия · Иркутск

ДМ

Дмитриев Алексей Владимирович

Научно-исследовательский институт ядерной физики им. Д.В. Скобельцина МГУ, Москва , Россия Россия · Москва

Факультет космических наук и инженерии, Национальный Центральный Университет, Тайвань Китайская Республика · Тайвань

СУ

Суворова Алла Васильевна

Ученая степень: кандидат физико-математических наук

Научно-исследовательский нститут ядерной физики им. Д.В. Скобельцина МГУ Россия · Москва

ХО

Хомутов Сергей Юрьевич

Ученая степень: кандидат физико-математических наук

Институт космофизических исследований и распространения радиоволн ДВО РАН Россия · Паратунка

ЦЭ

Цэгмэд Баттуулай

Ученая степень: кандидат физико-математических наук

Институт астрономии и геофизики АН Монголии Монголия · Улан-Батор

ТЕ

Теро Райта

Геофизическая обсерватория Соданкюля Финляндия · Соданкюля

АННОТАЦИЯ

We report the results of a study on the movement of the solar wind diamagnetic structure (DS), which is a sequence of smaller-scale microDS being part of the May 18, 2013 coronal mass ejection, from a source on the Sun to Earth’s surface. DS determined from the high negative correlation coefficient (r=–0.9) between the IMF modulus (B) and the SW density (N) on the ACE and Wind satellites at the L1 point, on the THB and THC satellites (r=–0.9) in near-Earth orbit, and on the THA satellite inside the magnetosphere is carried by the solar wind from the Sun to Earth’s orbit, while maintaining its fine internal structure. Having a large size in the radial direction (≈763 Rᴇ, where Rᴇ is the Earth radius), DS flows around the magnetosphere. At the same time, microDS of size ≤13 Rᴇ passes through the bow shock and magnetopause as a magnetized plasmoid in which the ion concentration increases from 10 cm⁻³ to 90 cm⁻³, and the velocity decreases as it moves toward the magnetotail. When a microDS passes through the magnetopause, a pulsed electric field of ~400 mV/m is generated with subsequent oscillations with a period of T~200 s and an amplitude of ~50 mV/m. The electric field accelerates charged particles of the radiation belt and produces modulated fluxes of protons in an energy range 95–575 keV on the day side and electrons in 40–475 keV and protons in 95–575 keV on the night side. In the duskside magnetosphere (19–23 MLT), the substorm activation is observed in geomagnetic pulsations and auroras, but without a magnetic negative bay. In the post-midnight sector (01–05 MLT), a sawtooth substorm occurs without the growth phase and breakup with deep modulation of the ionospheric current and auroral absorption. The duration of all phenomena in the magnetosphere and on Earth is determined by the period of interaction between DS and the magnetosphere (~4 hrs). To interpret the regularities of the magnetospheric response to the interaction with DS, we consider alternative models of the impulsive passage of DS from SW to the magnetosphere and the classical model of reconnection of IMF and the geomagnetic field.

КЛЮЧЕВЫЕ СЛОВА

diamagnetic structure, magnetized plasmoid, impulsive passage to the magnetosphere, sawtooth substorm

Финансирование

The work of Parkhomov V.A. was financially supported by the Ministry of Science and Higher Education of the Russian Federation under the project "Development of a mathematical model of the interaction between solar wind diamagnetic structures and Earth's magnetosphere" and by RFBR (Grant No. 18-55-52006 MNTa). The work of Eselevich V.G. and Eselevich M.G. was performed with budgetary funding of Basic Research program II.16. The work of Tsegmed B. was financially supported by the Academy of Sciences of Mongolia (Grant No. SHUAG_2017/17) and by the Ministry of Education, Science and Sports of Mongolia (project No. SHUSS-2017/65). The work of Khomutov S.Yu. was financially supported by the project "Physical processes in the system of near space and geospheres under solar and lithospheric effects", No. АААА-А21-121011290003-0.

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ГОСТ

Пархомов В. А., Еселевич В. Г., Еселевич М. В., Дмитриев А. В., Суворова А. В., Хомутов С. Ю., Цэгмэд Б., Теро Р. Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure // Solar-Terrestrial Physics. 2021. №. 3. С. 11-28. DOI: https://doi.org/10.12737/stp-73202102. (дата обращения: 23.09.2026).

MLA

Пархомов Владимир Александрович, Еселевич В. Г., Еселевич М. В., Дмитриев А. В., Суворова А. В., Хомутов С. Ю., Цэгмэд Б., Теро Р.. "Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure." Solar-Terrestrial Physics 7.3 (2021): 11-28. DOI: https://doi.org/10.12737/stp-73202102.

APA

Пархомов В. А., Еселевич В. Г., Еселевич М. В., Дмитриев А. В., Суворова А. В., Хомутов С. Ю., Цэгмэд Б., Теро Р. (2021). Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure. Solar-Terrestrial Physics, 7(3), 11-28. https://doi.org/10.12737/stp-73202102

Chicago

Пархомов Владимир Александрович, Еселевич В. Г., Еселевич М. В., Дмитриев А. В., Суворова А. В., Хомутов С. Ю., Цэгмэд Б., Теро Р.. "Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure." Solar-Terrestrial Physics 7, no. 3 (2021): 11-28. https://doi.org/10.12737/stp-73202102.

WIKI

{{cite journal | author = Пархомов В. А., Еселевич В. Г., Еселевич М. В., Дмитриев А. В., Суворова А. В., Хомутов С. Ю., Цэгмэд Б., Теро Р. | title = Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure | journal = Solar-Terrestrial Physics | year = 2021 | volume = 7 | issue = 3 | pages = 11-28 | doi = 10.12737/stp-73202102 }}

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MAGNETOSPHERIC RESPONSE TO THE INTERACTION WITH THE SPORADIC SOLAR WIND DIAMAGNETIC STRUCTURE Magnetospheric response to the interaction with the sporadic solar wind diamagnetic structure

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