Solnechno-Zemnaya Fizika Solnechno-Zemnaya Fizika Солнечно-земная физика 2712-9640 52318 10.12737/szf-91202306 Результаты исследований Results of current research Результаты исследований Electromagnetic ULF/ELF oscillations caused by the eruption of the Tonga volcano Электромагнитные УНЧ/КНЧ-колебания, вызванные извержением вулкана Тонга https://orcid.org/0000-0003-0734-6189 Мартинес-Беденко Валерий Армандович Martines-Bedenko Valery Armandovich lera_m0@mail.ru

кандидат физико-математических наук;

candidate of physical and mathematical sciences;

 https://orcid.org/0000-0003-3056-7465 Пилипенко Вячеслав Анатольевич Pilipenko Vyacheslav Anatolievich space.soliton@gmail.com

доктор физико-математических наук;

doctor of physical and mathematical sciences;

 Шиокава К. Shiokawa K. shiokawa@isee.nagoya-u.ac.jp https://orcid.org/0000-0002-6842-1552 Акбашев Ринат Рафикович Akbashev Rinat Rafikovich arr@emsd.ru

кандидат физико-математических наук;

candidate of physical and mathematical sciences;

 Институт физики Земли им. О.Ю. Шмидта РАН Москва Россия Schmidt Institute of Physics of the Earth RAS Moscow Russian Federation Институт физики Земли им. О.Ю. Шмидта РАН Москва Россия Schmidt Institute of Physics of the Earth RAS Moscow Russian Federation Геофизический центр РАН Москва Россия Geophysical Center RAS Moscow Russian Federation Институт космических исследований Москва Россия Space Research Institute Moscow Russian Federation Институт исследования околоземного пространства, Университет Нагойя Нагойя Япония Institute for Space–Earth Environmental Research, Nagoya University Nagoya Japan Камчатский филиал Единой геофизической службы РАН Петропавловск-Камчатский Россия Kamchatka Branch of the Unified Geophysical Survey RAS Petropavlovsk-Kamchatsky Russian Federation 28 03 2023 28 03 2023 9 1 51 59 06 08 2022 08 11 2022 https://naukaru.ru/en/nauka/article/52318/view

Извержение вулкана Тонга 13 и 15 января 2022 г. и сопровождавшая его интенсивная молниевая активность привели к возбуждению специфических электромагнитных колебаний разных частотных диапазонов. Свойства этих колебаний анализируются по данным магнитометров разных типов, расположенных на Камчатке и в Тихоокеанском регионе. Подтверждена возможность геомагнитного отклика на образование акустического резонанса между земной поверхностью и ионосферой: через ~15 мин после начала извержения на удалении ~800 км зарегистрированы локализованные гармонические колебания частотой 3.5–4.0 мГц, длившиеся ~1.5 ч. Отмечено усиление интенсивности шумановского резонанса (частота ~7.8 Гц) на станциях на Дальнем Востоке. Там же обнаружено появление широкополосного излучения в диапазоне Рс1 (2–5 Гц), стимулированного интенсивными вулканическими молниями. Это излучение, предположительно, является результатом возбуждения молниевой активностью магнитозвукового волновода в верхней ионосфере.

The eruption of the Tonga volcano on January 13 and 15, 2022 and related intense lightning activity led to the excitation of a number of specific electromagnetic oscillations in different frequency ranges. We examine properties of these oscillations, using data from magnetometers of various types located in Kamchatka and in the Pacific region. We confirmed that there might have been a geomagnetic response to the formation of an acoustic resonance between the Earth surface and the ionosphere: localized harmonic oscillations with a frequency 3.5–4.0 mHz, which lasted for ~1.5 hr, were detected ~15 min after the beginning of the eruption at distance of ~800 km. An increase was observed in the intensity of the Schumann resonance at stations in the Far East. Broadband emission stimulated by intense volcanic lightning was detected to occur in the Pc1 range (2–5 Hz). The emission presumably results from the excitation of the magnetosonic waveguide in the upper ionosphere by lightning activity.

 извержение вулкана атмосферные волны акустический резонанс шумановский резонанс Рс1 ионосферный волновод volcanic eruption atmospheric waves acoustic resonance Schumann resonance Pc1 ionospheric waveguide Работа поддержана грантом РНФ 22-17-00125 The work was financially supported by RSF (Grant No. 22-17-00125)

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