Solnechno-Zemnaya Fizika Solnechno-Zemnaya Fizika Солнечно-земная физика 2712-9640 47752 10.12737/szf-82202202 Результаты исследований Results of current research Результаты исследований Possible difference in the formation of coronal mass ejections of two types О возможном различии в формировании корональных выбросов массы двух типов Еселевич Виктор Григорьевич Eselevich Viktor Grigoryevich esel@iszf.irk.ru

доктор физико-математических наук;

doctor of physical and mathematical sciences;

 Еселевич Максим Викторович Eselevich Maxim Viktorovich mesel@iszf.irk.ru

кандидат физико-математических наук;

candidate of physical and mathematical sciences;

 https://orcid.org/0000-0001-6995-3684 Зимовец Иван Викторович Zimovets Ivan Victorovich

кандидат физико-математических наук;

candidate of physical and mathematical sciences;

 Институт солнечно-земной физики СО РАН Иркутск Россия Institute of Solar Terrestrial Physics SB RAS Irkutsk Russian Federation Институт солнечно-земной физики СО РАН Иркутск Россия Institute of Solar Terrestrial Physics SB RAS Irkutsk Russian Federation Институт космических исследований РАН Москва Россия Space Research Institute of RAS Moscow Russian Federation 30 06 2022 30 06 2022 8 2 12 22 16 12 2021 28 02 2022 https://zh-szf.ru/en/nauka/article/47752/view

Анализ семи окололимбовых корональных выбросов массы (КВМ) показал, что на расстояниях R<1.4R от центра Солнца по характеру формирования КВМ можно разделить на два типа. В случае КВМ типа 1 формирование фронтальной структуры (FS) происходит за счет процессов, протекающих внутри самой FS, представляющей собой внешнюю оболочку магнитного жгута. В случае КВМ типа 2 происходит эрупция внутренних арочных структур, которые взрывообразно расширяются, захватывают и ускоряют окружающие более удаленные арочные структуры, в результате слияния которых и формируется фронтальная структура КВМ типа 2.

Analysis of seven near-limb coronal mass ejections (CMEs) has shown that at distances R<1.4R from the center of the Sun CMEs according to their formation can be divided into two types: type 1 CMEs and type 2 CMEs. In the case of type 1 CMEs, the frontal structure (FS) is formed by processes occurring in FS itself, which is the outer shell of the magnetic flux rope. As for type 2 CMEs, EP-CME, internal arched structures erupt, explosively expand, capture and accelerate the more distant arched structures, which merge to form the frontal structure of the type 2 CMEs.

 корональный выброс массы магнитный жгут корональные арочные структуры вспышка эруптивный протуберанец coronal mass ejection magnetic flux rope coronal arched structures flare eruptive prominence Работа выполнена при финансовой поддержке Минобрнауки России (В.Г. Еселевич, М.В. Еселевич) и за счет субсидии в рамках гос. задания по теме «ПЛАЗМА» (И.В. Зимовец) The work was performed with financial support from the Ministry of Science and Higher Education of the Russian Federation (V.G. Eselevich, M.V. Eselevich) and under the Government Assignment "PLASMA" (I.V. Zimovets)

Еселевич В.Г., Еселевич М.В. Физические отличия в начальной фазе формирования двух типов корональных выбросов массы. Астрон. журн. 2014. Т. 91, № 4. С. 320-331. DOI: 10.7868/S0004629914030037. Alekseenko S.V., Dudnikova G.I., Romanov V.A., Romanov D.V., Romanov K.V. Magnetic field instabilities in the Solar convective zone. Russian J. Engineering Thermophysics. 2000, vol. 10, pp. 243-262. Еселевич В.Г., Еселевич М.В. Особенности начальной стадии формирования быстрого коронального выброса массы 25 февраля 2014 г. Солнечно-земная физика. 2020. Т. 6, № 3. С. 3-17. DOI: 10.12737/szf-63202001. Amari T., Luciani J.F., Mikic Z., Linker J. A twist flux rope model for coronal mass ejections and two-ribbon flare. Astrophys. J. 2000, vol. 529, pp. L49-L52. DOI: 10.1086/312444. Еселевич В.Г., Еселевич М.В., Романов В.А. и др. Физический механизм генерации корональных выбросов массы из верхних слоев конвективной зоны. Изв. Крымской астрофиз. обс. 2013. Т. 109, № 4. С. 54-60. Antiochos S.K., DeVore C.R., Klimchuk J.A. A model for solar coronal mass ejections. Astrophys. J. 1999, vol. 510, pp. 485-493. DOI: 10.1086/306563. Еселевич В.Г., Еселевич М.В., Зимовец И.В., Руденко Г.В. Исследование начальной стадии формирования импульсного коронального выброса массы. Астрон. журн. 2016. Т. 93, № 11. С. 990-1002. DOI: 10.7868/S0004629916100029. Archontis V., Hood A.W. A flux emergence model for solar eruptions. Astrophys. J. 2008, vol. 674, pp. L113-L116. DOI: 10.1086/529377. Романов В.А., Романов Д.В., Романов К.В. Сброс магнитных полей из зоны действия солнечного динамо в атмосферу Солнца. Астрон. журн. 1993а. Т. 70. С. 1237-1246. Bemporad A., Raymond J., Poletto G., Romoli M. A comprehensive study of the initiation and early evolution of a coronal mass ejection from ultraviolet and white-light data. Astrophys. J. 2007, vol. 655, pp. 576-590. DOI: 10.1086/509569. Романов В.А., Романов Д.В. Романов К.В. Сброс магнитных полей из зоны действия солнечного динамо в релаксационную зону. Астрон. журн. 1993б. Т. 70. P. 1247-1256. Chen H., Zhang J., Cheng X., Ma S., Yang S., Li T. Direct observations of tether-cutting reconnection during a major solar event from 2014 February 24 to 25. Astrophys. J. Lett. 2014, vol. 797, article id. L15. Alekseenko S.V., Dudnikova G.I., Romanov V.A., et al. Magnetic field instabilities in the Solar convective zone. Russian J. Engineering Thermophysics. 2000. Vol. 10. P. 243-262. Eselevich V.G., Eselevich M.V. On the Formation Mechanism of the Sporadic Solar Wind. Geomagnetism and Aeronomy. 2011, vol. 51, no. 8, pp. 1083-1094. Amari T., Luciani J.F., Mikic Z., Linker J. A twist flux rope model for coronal mass ejections and two-ribbon flare. Astrophys. J. 2000. Vol. 529. P. L49-L52. DOI: 10.1086/312444. Eselevich V.G., Eselevich M.V., Romanov V.A., Romanov D.V., Romanov K.V., Kucherov N.V. Physical mechanism for the generation of the coronal mass ejections from the upper layers of the convective zone. Izvestiya Krymskoj Astrofizicheskoj Observatorii. 2013, vol. 109, no. 4, pp. 54-60. (In Russian). Antiochos S.K., DeVore C.R., Klimchuk J.A. A model for solar coronal mass ejections. Astrophys. J. 1999. Vol. 510. P. 485-493. DOI: 10.1086/306563. Eselevich V.G., Eselevich M.V. Physical differences between the initial phase of the formation of two types of coronal mass ejections. Astronomicheskii Zhurnal [Astronomy Reports]. 2014, vol. 91, no. 4, pp. 320-331. (In Russian). Archontis V., Hood A.W. A flux emergence model for solar eruptions. Astrophys. J. 2008. Vol. 674. P. L113-L116. DOI: 10.1086/529377. Eselevich V.G., Eselevich M.V., Zimovets I.V., Rudenko G.V. Study of the initial formation stage of an impulsive coronal mass ejection. Astronomicheskii Zhurnal [Astronomy Reports]. 2016, vol. 93, no. 11, pp. 990-1002. (In Russian). Bemporad A., Raymond J., Poletto G., Romoli M. A comprehensive study of the initiation and early evolution of a coronal mass ejection from ultraviolet and white-light data. Astrophys. J. 2007. Vol. 655. P. 576-590. DOI: 10.1086/509569. Eselevich V.G., Eselevich M.V. Features of the initial stage of formation of fast coronal mass ejection on February 25, 2014. Solnechno-Zemnaya Fizika [Solar-Terrestrial Physics]. 2020, vol. 6, no. 3, pp. 3-17. (In Russian). Chen H., Zhang J., Cheng X., Ma S., et al. Direct observations of tether-cutting reconnection during a major solar event from 2014 February 24 to25. Astrophys. J. Lett. 2014. Vol. 797, article id. L15. DOI: 10.1088/2041-8205/797/2/L15. Gibson S. E., Foster D., Burkepile J., de Toma G., Stanger A. The calm before the storm: the link between quiescent cavities and coronal mass ejections. Astrophys. J. 2006, vol. 641. pp. 590-605. DOI: 10.1086/500446. Eselevich V.G., Eselevich M.V. On the formation mechanism of the sporadic solar wind. Geomagnetism and Aeronomy. 2011. Vol. 51, no. 8. P. 1083-1094. Hundhausen A.J. Coronal mass ejections. The Many Faces of the Sun: A Summary of the Results from NASA’s Solar Maximum Mission. New York, Springer, 1999, pp. 143-200. Gibson S.E., Foster D., Burkepile J., et al. The calm before the storm: the link between quiescent cavities and coronal mass ejections. Astrophys. J. 2006. Vol. 641. P. 590-605. DOI: 10.1086/500446. Kliem B., Titov V.S., Török T. Formation of current sheets and sigmoidal structure by the kink instability of a magnetic loop. Astron. Astrophys. 2004, vol. 413, pp. L23-L26. DOI: 10.1051/0004-6361:20031690. Hundhausen A.J. Coronal mass ejections: A summary of SMM observations from 1980 and 1984-1989. The Many Faces of the Sun: A Summary of the Results from NASA’s Solar Maximum Mission. New York, Springer, 1999. P. 143-200. Kliem B., Török T. Torus instability. Phys. Rev. Lett. 2006, vol. 96, iss. 25, id. 255002. DOI: 10.1103/PhysRevLett.96.255002. Kliem B., Titov V.S., Török T. Formation of current sheets and sigmoidal structure by the kink instability of a magnetic loop. Astron. Astrophys. 2004. Vol. 413. P. L23-L26. DOI: 10.1051/0004-6361:20031690. Krall J., Chen J., Santoro R. Drive mechanisms of erupting solar magnetic flux ropes. Astrophys. J. 2000, vol. 539, pp. 964-982. DOI: 10.1086/309256. Kliem B., Török T. Torus Instability. Phys. Rev. Lett. 2006. Vol. 96, iss. 25, id. 255002. DOI: 10.1103/PhysRevLett. 96.255002. Lemen J.R., Title A.M., Akin D.J., Boerner P.F., Chou C., Drake J.F., Duncan D.W., et al. The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO). Solar Phys. 2012, vol. 275, iss. 1-2, pp. 17-40. DOI: 10.1007/s11207-011-9776-8. Krall J., Chen J., Santoro R. Drive mechanisms of erupting solar magnetic flux ropes. Astrophys. J. 2000. Vol. 539. P. 964-982. DOI: 10.1086/309256. MacQueen R.N., Fisher R.R. The kinematic of solar inner coronal transient. Solar Phys. 1983, vol. 89, pp. 89-102. DOI: 10.1007/BF00211955. Lemen J.R., Title A.M., Akin D.J., et al. The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO). Solar Phys. 2012. Vol. 275, iss. 1-2. P. 17-40. DOI: 10.1007/s11207-011-9776-8. Magara T., Longcope D.W. Sigmoid structure of an emerging flux tube. Astrophys. J. 2001, vol. 559, iss. 1, pp. L55-L59. DOI: 10.1086/323635. MacQueen R.N., Fisher R.R. The kinematic of solar inner coronal transient. Solar Phys. 1983. Vol. 89. P. 89-102. DOI: 10.1007/BF00211955. Moore R.L., Sterling A.C., Hudson H.S., Lemen J.R. onset of the magnetic explosion in solar flares and coronal mass ejections. Astrophys. J. 2001, vol. 552, pp. 833-848. DOI: 10.1086/320559. Magara T., Longcope D.W. Sigmoid structure of an emerging flux tube. Astrophys. J. 2001. Vol. 559, iss. 1. P. L55-L59. DOI: 10.1086/323635. Moreno-Insertis F., Schussler M., Ferriz-Mas A. Storage of magnetic flux tubes in a convective overshoot. Astron. Astrophys. 1992, vol. 264, pp. 686-700. Moore R.L., Sterling A.C., Hudson H.S., Lemen J.R. Onset of the magnetic explosion in solar flares and coronal mass ejections. Astrophys. J. 2001. Vol. 552. P. 833-848. DOI: 10.1086/320559. Patsourakos S., Vourlidas A., Stenborg G. Direct evidence for a fast coronal mass ejection driven by the prior formation and subsequent destabilization of a magnetic flux rope. Astrophys. J. 2013, vol. 764, article id. 125. DOI: 10.1088/0004-637X/764/2/125. Moreno-Insertis F., Schussler M., Ferriz-Mas A. Storage of magnetic flux tubes in a convective overshoot. Astron. Astrophys. 1992. Vol. 264. P. 686-700. Romanov V.A., Romanov D.V., Romanov K.V. Fault of magnetic fields from the dynamo action region into the atmosphere of the Sun. Astronomicheskii Zhurnal [Astronomy Reports]. 1993a, vol. 70, pp. 1237-1246. (In Russian). Patsourakos S., Vourlidas A., Stenborg G. Direct evidence for a fast coronal mass ejection driven by the prior formation and subsequent destabilization of a magnetic flux rope. Astrophys. J. 2013. Vol. 764, article id. 125. DOI: 10.1088/0004-637X/764/2/125. Romanov V.A., Romanov D.V., Romanov K.V. Fault of magnetic fields from the solar dynamo action region into the relaxation zone. Astronomicheskii Zhurnal [Astronomy Reports]. 1993b, vol. 70, pp. 1247-1256. (In Russian). Schmieder B., Démoulin P., Aulanier G. Solar filament eruptions and their physical role in triggering coronal mass ejections. Adv. Space Res. 2013. Vol. 51. P. 1967-1980. DOI: 10.1016/j.asr.2012.12.026. Schmieder B., Démoulin P., Aulanier G. Solar filament eruptions and their physical role in triggering coronal mass ejections. Adv. Space Res. 2013, vol. 51, pp. 1967-1980. DOI: 10.1016/j.asr.2012.12.026. Sharykin I.N., Zimovets I.V., Myshyakov I.I. Flare Energy Release at the Magnetic Field Polarity Inversion Line during the M1.2 Solar Flare of 2015 March 15. II. Investigation of Photospheric Electric Current and Magnetic Field Variations Using HMI 135 s Vector Magnetograms. Astrophys. J. 2020. Vol. 893, iss. 2, 159. DOI: 10.3847/1538-4357/ab84ef. Sharykin I.N., Zimovets I.V., Myshyakov I.I. Flare Energy Release at the Magnetic Field Polarity Inversion Line during the M1.2 Solar Flare of 2015 March 15. II. Investigation of Photospheric Electric Current and Magnetic Field Variations Using HMI 135 s Vector Magnetograms. Astrophys. J. 2020, vol. 893, iss. 2, 159. DOI: 10.3847/1538-4357/ab84ef. Sheeley N.R.Jr., Walters J.H., Wang Y.-M., Howard R.A. Continuous tracking of coronal outflows: Two kinds of coronal mass ejections. J. Geophys. Res. 1999. Vol. 104, no. A11. P. 24739-24768. DOI: 10.1029/1999JA900308. Sheeley N.R. Jr., Walters J.H., Wang Y.-M., Howard R.A. Continuous tracking of coronal outflows: Two kinds of coronal mass ejections. J. Geophys. Res. 1999, vol. 104, no. A11, pp. 24739-24768. DOI: 10.1029/1999JA900308. Shen Y., Liu Y., Su J. Sympathetic partial and full filament eruptions observed in one solar breakout event. Astrophys. J. 2012. Vol. 750, article id. 12. DOI: 10.1088/0004-637X/750/1/12. Shen Y., Liu Y., Su J. Sympathetic partial and full filament eruptions observed in one solar breakout event. Astrophys. J. 2012, vol. 750, article id. 12. DOI: 10.1088/0004-637X/750/1/12. Sterling A.C., Moore R.L. Slow-Rise and Fast-Rise Phases of an Erupting Solar Filament, and Flare Emission Onset. Astrophys. J. 2005. Vol. 630. P. 1148-1159. DOI: 10.1086/432044. Sterling A.C., Moore R.L. Slow-rise and fast-rise phases of an erupting solar filament, and flare emission onset. Astrophys. J. 2005, vol. 630, pp. 1148-1159. DOI: 10.1086/432044. Thernisien A., Vourlidas A., Howard R.A. Forward modeling of Coronal Mass Ejection using STEREO/SECCHI data. Solar Phys. 2009. Vol. 256. P. 111-130. DOI: 10.1007/s11207-009-9346-5. Thernisien A., Vourlidas A., Howard R.A. Forward modeling of Coronal Mass Ejection using STEREO/SECCHI data. Solar Phys. 2009, vol. 256, pp. 111-130. DOI: 10.1007/s11207-009-9346-5. Vršnak, B., Sudar D., Ruzdjak D. The CME-flare relationship: Are there really two types of CME? Astron. Astrophys. 2005. Vol. 435. P. 1149-1109. DOI: 10.1051/0004-6361: 20042166. Vršnak, B., Sudar D., Ruzdjak D. The CME-flare relationship: Are there really two types of CME? Astron. Astrophys. 2005, vol. 435, pp. 1149-1109. DOI: 10.1051/0004-6361: 20042166. Zhang J., Wang J., Deng Y., Wu D. Magnetic flux cancellation associated with the major solar event on 2000 July 14. Astrophys. J. 2001. Vol. 548. P. L99-L102. DOI: 10.1086/318934. Zhang J., Wang J., Deng Y., Wu D. Magnetic Flux Cancellation Associated with the Major Solar Event on 2000 July 14. Astrophys. J. 2001, vol. 548, pp. L99-L102. DOI: 10.1086/318934. Zhang J., Dere K.P. A statistical study of main and residual accelerations of Coronal Mass Ejections. Astrophys. J. 2006. Vol. 649. P. 1100-1109. DOI: 10.1086/506903. Zhang J., Dere K.P. A statistical study of main and residual accelerations of coronal mass ejections. Astrophys. J. 2006, vol. 649, pp. 1100-1109. DOI: 10.1086/506903. URL: http://cdaw.gsfc.nasa.gov/CME_list (дата обращения 15 декабря 2021 г.). URL: http://cdaw.gsfc.nasa.gov/CME_list (accessed December 15, 2021).