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Особенности короткопериодических колебаний микроволнового излучения активной области Солнца перед вспышкой.
С. 15–18.
Абрамов-Максимов В. Е., Bakunina I. A.
In book
СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2017.
Bakunina I. A., Мельников В. Ф., Шаин А. В. et al., Геомагнетизм и аэрономия 2025 Т. 65 № 9 С. 1363–1373
Рассмотрена связь особенностей положения и ориентации магнитных жгутов в активной области (АО) с источниками микроволнового (17 ГГц) излучения и излучения в крайнем ультрафиолетовом диапазоне (EUV) при возникновении эруптивных вспышек, сопровождающихся корональными выбросами массы, и вспышек с "запертой" эрупцией. Приведены примеры эруптивных событий, демонстрирующие пространственное совпадение микроволновых источников с расположением магнитных жгутов в АО, восстановленных при ...
Added: June 22, 2026
I. A. Bakunina, Melnikov V. F., Shain A. V. et al., Geomagnetism and Aeronomy 2024 Vol. 64 No. 8 P. 1237–1249
Using statistics from 15 X-ray class M flare events, the features of the position and orientation of magnetic flux ropes in the general spatial structure of the magnetic field of the active region (AR) during flares and coronal mass ejections (CME) were studied by reconstructing the coronal magnetic field from the photosphere to the corona ...
Added: February 17, 2025
Abramov-Maximov V. E., Bakunina I. A., Geomagnetism and Aeronomy 2024 Vol. 64 No. 7 P. 1054–1058
For the first time, several flare events are analyzed based on multifrequency observations using the
Radio Solar Telescope Network. The purpose of the analysis is to identify signs of flare preparation. In all
considered cases, preflare quasi-periodic fluctuations (QPFs) of radio emission were detected. The duration of
preflare wavetrains is 6–20 min. Wavetrains consist of 3–5 pulses. QPFs ...
Added: February 17, 2025
Bakunina I. A., Мельников В. Ф., Шаин А. В. et al., В кн.: XXVIII всероссийская ежегодная конференция «Солнечная и солнечно-земная физика-2024», Труды.: СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2024. С. 25–28.
It is shown on a sample of 15 M-class X-ray flares that CMEs occur in events with «open» magnetic ropes reconstructed in the NLFFF approximation. Magnetic ropes coincide with radio brightness maxima at 17 GHz. Several hours before the flare, in the region of magnetic ropes, a glow of loops in the EUV (94, 131 ...
Added: December 1, 2024
СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2024.
Сборник содержит доклады, представленные на XXVIII Всероссийскую ежегодную конференцию по физике Солнца «Солнечная и солнечно-земная физика – 2024» (7 – 11 октября 2024, ГАО РАН, Санкт-Петербург). Конференция проводилась Главной (Пулковской) астрономической обсерваторией РАН при поддержке секции «Солнце» Научного совета по астрономии РАН и секции «Физика солнечной плазмы» Научного совета «Солнце-Земля». Тематика конференции включала в себя ...
Added: December 1, 2024
I. A. Bakunina, Melnikov V. F., Kuznetsov S. A. et al., Geomagnetism and Aeronomy, Netherlands 2023 Vol. 63 No. 8 P. 1154–1166
The dynamics of the magnetic field reconstructed in the nonlinear force-free approximation in the pre-flare and post-flare phases of M-class X-ray flares in seven active regions is considered: two flares with a coronal mass ejection (CME), two flares with eruption but no CMEs, and three flares without eruption. Extrapolation of the magnetic field to the ...
Added: February 3, 2024
Abramov-Maximov V. E., I. A. Bakunina, Geomagnetism and Aeronomy, Springer, Switzerland 2023 Vol. 63 No. 7 P. 916–919
We present a study of the frequency of occurrence of quasi-periodic fluctuations (QPFs) of microwave
radiation from solar active regions at the pre-flare stage. We used correlation curves obtained with the
Nobeyama Radioheliograph (NoRH). We analyzed 529 flares of classes X, M, and C (according to the GOES
classification). In a significant number of considered events (approximately 75% ...
Added: December 28, 2023
P.A.Bespalov, O.N.Savina, Geomagnetism and Aeronomy 2023 Vol. 63 No. 7 P. 910–915
According to modern concepts, Type I noise storms in the meter wavelength range (30–400 MHz), consisting of a large number of narrow-band short bursts, are excited in the rarefied solar corona. These radiations are characterized by a high brightness temperature and circular polarization. Despite many advances in theory and confidence that the mechanism of radiation ...
Added: December 22, 2023
Bakunina I. A., Мельников В. Ф., Шаин А. В. et al., В кн.: Труды XXVII Всероссийской ежегодной конференции по физике Солнца “Солнечная и солнечно-земная физика - 2023”, 9-13 октября 2023 года, Санкт-Петербург, ГАО РАН.: СПб.: ГАО РАН, 2023. С. 23–26.
It is shown that the positions of the flux ropes in the general spatial structure of the active region magnetic field reconstructed in the NLFFF approximation for flares with and without CME are different: magnetic flux ropes are located quasi-parallel to the overlying magnetic field lines in the events with CME, and quasi-perpendicular in the ...
Added: December 3, 2023
I. A. Bakunina, Melnikov V. F., Shain A. V. et al., Geomagnetism and Aeronomy 2022 Vol. 62 No. 8 P. 1066–1072
The dynamics of the preflare phase of microwave and ultraviolet emission for M-class X-ray flares in three active regions (ARs), two flares with coronal mass ejections (CMEs) and one flare without a CME, were considered. Extrapolation of the magnetic field in the AR corona showed that eruptive events were associated with the formation of a ...
Added: February 16, 2023
Abramov-Maximov V. E., I. A. Bakunina, Geomagnetism and Aeronomy 2022 Vol. 62 No. 7 P. 895–902
We present a study of the spatial distribution of quasi-periodic oscillations (QPOs) of microwave emission in three solar active regions before flares. The following events are considered: SOL2011-09-06T01:50M5.3, SOL2011-09-25T02:33M4.4, and SOL2012-07-08T04:19C6.6. Daily observations on the Nobeyama Radioheliograph at a frequency of 17 GHz are used. In all three cases, pre-flare trains of the QPOs of ...
Added: February 16, 2023
Абрамов-Максимов В. Е., Bakunina I. A., В кн.: Труды XXVI Всероссийской ежегодной конференции по физике Солнца “Солнечная и солнечно-земная физика - 2022, 3-7 октября 2022.: СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2022. С. 9–12.
Added: February 11, 2023
И. А. Бакунина, В.Ф. М., В.Е. А., В кн.: Труды XXVI Всероссийской ежегодной конференции по физике Солнца “Солнечная и солнечно-земная физика - 2022, 3-7 октября 2022.: СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2022. С. 17–20.
Reconstruction of the magnetic field in a nonlinear force-free approximation based on SDO/HMI vector magnetograms for X-ray class M flares, some of which were accompanied by coronal mass ejections (CME), allowed to reveal different stages of the formation of magnetic ropes in the flare region. Based on SDO/HMI observations, as well as on the Nobeyama ...
Added: February 11, 2023
Bakunina I. A., Мельников В. Ф., Шаин А. В. et al., Известия Крымской астрофизической обсерватории 2022 Т. 118 № 1 С. 65–74
To date, observational signs that determine the ability of solar active region to cause an eruption of matter into the high layers of the solar corona (CME) are not entirely clear. This makes it difficult to understand the physical mechanism of the CME trigger. This paper presents a search for observational signs that may indicate ...
Added: March 23, 2022
Bakunina I. A., Мельников В. Ф., Шаин А. В. et al., В кн.: Труды XXV Всероссийской ежегодной конференции по физике Солнца “Солнечная и солнечно-земная физика - 2021, 4-8 октября 2021, ГАО РАН.: СПб.: ГАО РАН, 2021. С. 47–50.
The dynamics of microwave and EUV emission is considered for active regions with CME and with no eruption. Extrapolation of the magnetic field to the corona of active region (AR) has shown that an eruption event may be connected with the presence of a twisted magnetic field and an open magnetic configuration in the flare ...
Added: February 2, 2022
СПб.: ГАО РАН, 2021.
Сборник содержит доклады, представленные на XXV Всероссийскую ежегодную конференцию по физике Солнца «Солнечная и солнечно-земная физика – 2021» (4 – 8 октября 2021, ГАО РАН, Санкт-Петербург). Конференция проводилась Главной (Пулковской) астрономической обсерваторией РАН при поддержке секции «Солнце» Научного совета по астрономии РАН и секции «Плазменные процессы в магнитосферах планет, атмосферах Солнца и звёзд» Научного совета ...
Added: February 2, 2022
Bakunina I. A., Melnikov V. F., Abramov-Maximov V. E. et al., Geomagnetism and Aeronomy 2021 Vol. 61 No. 8 P. 1159–1171
In this study, a comparative analysis was carried out on the preflare and flare conditions for six flares accompanied by coronal mass ejections (CMEs) and five events not accompanied by CMEs. All of the events occurred in the period 2011–2014. The features of the spatial dynamics of microwave emission of active regions (data from the ...
Added: October 29, 2021
Bakunina I. A., Мельников В. Ф., Абрамов-Максимов В. Е. et al., В кн.: Труды XXIV Всероссийской ежегодной конференции по физике Солнца “Солнечная и солнечно-земная физика - 2020, 5-9 октября 2020, ГАО РАН.: СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2020. С. 15–18.
Solar flares and coronal mass ejections (CME) are the most powerful manifestations of solar activity. Both phenomena associated with the evolution of the spatial structure of the magnetic field of active regions (AR). It is known that not all powerful flares accompanied by CME. In some cases, CME are observed, associated with very low intensity ...
Added: January 18, 2021
СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2020.
Сборник содержит доклады, представленные на XXIV Всероссийскую ежегодную конференцию по физике Солнца «Солнечная и солнечно-земная физика – 2020» (5 – 9 октября 2020, ГАО РАН, Санкт-Петербург). Конференция проводилась Главной (Пулковской) астрономической обсерваторией РАН при поддержке секции «Солнце» Научного совета по астрономии РАН и секции «Плазменные процессы в магнитосферах планет, атмосферах Солнца и звёзд» Научного совета ...
Added: January 18, 2021
Abramov-Maximov V. E., Bakunina I. A., Geomagnetism and Aeronomy 2020 Vol. 60 No. 7 P. 846–852
A study of quasi-periodic fluctuations of solar microwave emission at the pref lare stage is pre-sented. Data from daily solar observations by the Nobeyama Radioheliograph at a frequency of 17 GHz areused. Five f lares are analyzed based on synthesized two-dimensional radio images. All of the consideredevents are characterized by pref lare fluctuations of microwave emission ...
Added: January 18, 2021
Bakunina I. A., Melnikov V. F., Morgachev A. S., Geomagnetism and Aeronomy 2020 Vol. 60 No. 7 P. 853–859
The spatial dynamics of microwave emission (data from the Nobeyama Radioheliograph) of activeregions with a complex magnetic field configuration before powerful f lares, as well as the fine structure ofactive sources of ultraviolet (UV) emission based on AIA/SDO data, are studied. It is shown that there isunsteady behavior of microwave sources, along with the ignition ...
Added: January 18, 2021