Solar-Terrestrial Physics Solar-Terrestrial Physics Solar-Terrestrial Physics 2500-0535 103580 10.12737/stp-113202502 20TH ANNUAL CONFERENCE “PLASMA PHYSICS IN THE SOLAR SYSTEM”. FEBRUARY 10–14, 2025, SPACE RESEARCH INSTITUTE RAS, MOSCOW, RUSSIA 20TH ANNUAL CONFERENCE “PLASMA PHYSICS IN THE SOLAR SYSTEM”. FEBRUARY 10–14, 2025, SPACE RESEARCH INSTITUTE RAS, MOSCOW, RUSSIA 20TH ANNUAL CONFERENCE “PLASMA PHYSICS IN THE SOLAR SYSTEM”. FEBRUARY 10–14, 2025, SPACE RESEARCH INSTITUTE RAS, MOSCOW, RUSSIA Features of turbulent cascade development in the magnetosheath during ICME Features of turbulent cascade development in the magnetosheath during ICME Рахманова Людмила Сергеевна Rakhmanova Liudmila Sergeevna rakhlud@gmail.com

кандидат физико-математических наук;

candidate of physical and mathematical sciences;

 Рязанцева Мария Олеговна Riazantseva Maria Olegovna orearm@gmail.com Хохлачев Александр Андреевич Khokhlachev Aleksander Andreevich aleks.xaa@yandex.ru Ермолаев Юрий Иванович Yermolaev Yuri Ivanovich yermol@iki.rssi.ru

доктор физико-математических наук;

doctor of physical and mathematical sciences;

 Застенкер Георгий Наумович Zastenker Georgy Naumovich gzastenk@iki.rssi.ru

доктор физико-математических наук;

doctor of physical and mathematical sciences;

 Институт космических исследований РАН Москва Россия Space Research Institute RAS Moscow Russian Federation Институт космических исследований РАН Москва Россия Space Research Institute of RAS (IKI) Moscow Russian Federation Институт космических исследований РАН Москва Россия Space Research Institute RAS Moscow Russian Federation Институт космических исследований РАН Москва Россия Space Research Institute RAS Moscow Russian Federation Институт космических исследований РАН Москва Россия Space Research Institute RAS Moscow Russian Federation 22 09 2025 22 09 2025 11 3 13 21 10 03 2025 05 05 2025 https://naukaru.ru/en/nauka/article/103580/view

Large-scale disturbances in the interplanetary medium are the main cause of the global perturbations inside Earth’s magnetosphere. Transition region called magnetosheath is known to be located in front of the magnetosphere in which plasma and magnetic field properties, as well as their variations differ significantly from those in the solar wind. Particularly, plasma passage through the magnetosheath has been demonstrated to modify substantially features of the cascade of turbulent fluctuations of the solar wind, with the pattern of the modification being different for quiet and disturbed conditions in the interplanetary medium. In this study, we examine features of turbulent cascade formation in the magnetosheath during interplanetary manifestation of coronal mass ejection (ICME), by analyzing several cases of ICME interactions with the magnetosphere. The analysis is conducted by comparing magnetic field variations measured simultaneously in the solar wind and in the dayside magnetosheath by Wind, Cluster, THEMIS, and MMS spacecraft in 2016–2017. Interaction of ICME with the magnetosphere is shown to cause the least change in the fluctuation power if there is a compression region in front of it; on the opposite, when there is no compression region, the fluctuation power increases considerably. ICMEs that caused significant changes in the Dst index were determined to be accompanied by the least changes in the turbulent cascade in the magnetosheath, whereas the most significant modification of the turbulence features were observed during ICMEs which did not trigger substantial geomagnetic disturbances

Large-scale disturbances in the interplanetary medium are the main cause of the global perturbations inside Earth’s magnetosphere. Transition region called magnetosheath is known to be located in front of the magnetosphere in which plasma and magnetic field properties, as well as their variations differ significantly from those in the solar wind. Particularly, plasma passage through the magnetosheath has been demonstrated to modify substantially features of the cascade of turbulent fluctuations of the solar wind, with the pattern of the modification being different for quiet and disturbed conditions in the interplanetary medium. In this study, we examine features of turbulent cascade formation in the magnetosheath during interplanetary manifestation of coronal mass ejection (ICME), by analyzing several cases of ICME interactions with the magnetosphere. The analysis is conducted by comparing magnetic field variations measured simultaneously in the solar wind and in the dayside magnetosheath by Wind, Cluster, THEMIS, and MMS spacecraft in 2016–2017. Interaction of ICME with the magnetosphere is shown to cause the least change in the fluctuation power if there is a compression region in front of it; on the opposite, when there is no compression region, the fluctuation power increases considerably. ICMEs that caused significant changes in the Dst index were determined to be accompanied by the least changes in the turbulent cascade in the magnetosheath, whereas the most significant modification of the turbulence features were observed during ICMEs which did not trigger substantial geomagnetic disturbances

 solar wind magnetosheath turbulence space plasma solar wind magnetosheath turbulence space plasma The work was carried out under the Government assignment from IKI RAS on the theme “PLASMA” The work was carried out under the Government assignment from IKI RAS on the theme “PLASMA”

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