Библиография

1. 1. Прист Э., Форбс Т. Магнитное пересоединение. Пер. с англ. ред. В.Д. Кузнецов, А.Г. Франк. М: Физматлит, 592 с. 2005.
2. 2. Carmichael H. A process for flares / The Physics of Solar Flares / Proceedings of the AAS-NASA Symposium. Greenbelt, MD. October 28−30, 1963. Ed. Hess W.N. SP-50 of NASA Special Publications, Washington: NASA Scientific and Technical Information Division. P. 451−456. 1964.
3. 3. Carrington R.C. Description of a singular appearance seen in the Sun on September 1, 1859 // Mon. Not. R. Astron. Soc. V. 20. P. 13−15. 1859.
4. 4. Ding M.D., Chen Q.R., Li J.P., Chen P.F. Hα and hard X-ray observations of a two-ribbon flare associated with a filament eruption // Astrophys. J. V. 598. № 1. P. 683−688. 2003. https://doi.org/10.1086/378877
5. 5. Durant C.J. Polar magnetic fields – filaments and the zero-flux contour // Solar Phys. V. 211. № 1−2. P. 83−102. 2002. https://doi.org/10.1023/A:1022501505915
6. 6. Filippov B. Electric current equilibrium in the corona // Solar Phys. V. 283. № 2. P. 401−411. 2013. https://doi.org/10.1007/s11207-013-0253-4
7. 7. Filippov B. Rising of a magnetic null point in the wake of an erupting flux rope // Mon. Not. R. Astron. Soc. V. 512. № 1. P. 1357–1364. 2022. https://doi.org/10.1093/mnras/stac575
8. 8. Fletcher L., Dennis B.R., Hudson H.S. et al. An observational overview of solar flares // Space Sci. Rev. V. 159. № 1−4. ID 19. 2011. https://doi.org/10.1007/s11214-010-9701-8
9. 9. Forbes T.G., Priest E.R. Reconnection in solar flares / Solar Terrestrial Physics: Present and Future. Eds. Butler D.M., Papadopoulous K. Greenbelt, MD: NASA Reference Publication 1120. P. 1−35. 1984.
10. 10. Forbes T.G., Lin J. What can we learn about reconnection from coronal mass ejections? // J. Atmos. Sol.-Terr. Phy. V. 62. № 16. P. 1499−1507. 2000. https://doi.org/10.1016/S1364-6826 (00)00083-3
11. 11. Forbes T.G., Seaton D.B., Reeves K.K. Reconnection in the post-impulsive phase of solar flares // Astrophys. J. V. 858. № 2. ID 70. 2018. https://doi.org/10.3847/1538-4357/aabad4
12. 12. Hinterreiter J., Veronig A.M., Thalmann J.K., Tschernitz J., Pötzi W. Statistical properties of ribbon evolution and reconnection electric fields in eruptive and confined flares // Solar Phys. V. 293. № 3. ID 38. 2018. https://doi.org/10.1007/s11207-018-1253-1
13. 13. Hirayama T. Theoretical model of flares and prominences. I: Evaporating flare model // Solar Phys. V. 34. № 2. P. 323−338. 1974. https://doi.org/10.1007/BF00153671
14. 14. Kopp R.A., Pneuman G.W. Magnetic reconnection in the corona and the loop prominence phenomenon // Solar Phys. V. 50. № 1. P. 85−98. 1976. https://doi.org/10.1007/BF00206193
15. 15. Kuperus M., Raadu M.A. The support of prominences formed in neutral sheets // Astron. Astrophys. V. 31. P. 189−193. 1974.
16. 16. Lemen J.R., Title A.M., Akin D.J., et al. The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO) // Solar Phys. V. 275. № 1−2. P. 17−40. 2012. https://doi.org/10.1007/s11207-011-9776-8
17. 17. Li L., Zhang J. On the brightening propagation of post-flare loops observed by TRACE // Astrophys. J. V. 690. № 1. P. 347−357. 2009. https://doi.org/10.1088/0004-637X/690/1/347
18. 18. Lin J., Forbes T.G., Isenberg P.A., Démoulin P. The effect of curvature on flux-rope models of coronal mass ejections // Astrophys. J. V. 504. № 2. P. 1006−1019. 1998. https://doi.org/10.1086/306108
19. 19. Lin J., Soon W., Baliunas S.L. Theories of solar eruptions: a review // New Astron. Rev. V. 47. № 2. P. 53−84. 2003. https://doi.org/10.1016/S1387-6473 (02)00271-3
20. 20. Martin S.F. Conditions for the formation and maintenance of filaments (invited review) // Solar Phys. V. 182. № 1. P. 107−137. 1998. https://doi.org/10.1023/A:1005026814076
21. 21. McIntosh P.S. Solar magnetic fields derived from hydrogen alpha filtergrams // Rev. Geophys. Space Phys. V. 10. № 3. P. 837−846. 1972. https://doi.org/10.1029/RG010i003p00837
22. 22. Priest E.R., Forbes T.G. Magnetic field evolution during prominence eruptions and two-ribbon flares // Solar Phys. V. 126. № 2. P. 319−350. 1990. https://doi.org/10.1007/BF00153054
23. 23. Priest E.R., Forbes T.G. The magnetic nature of solar flares // Astron. Astrophys. Rev. V. 10. № 4. P. 313−377. 2002. https://doi.org/10.1007/s001590100013
24. 24. Qiu J., Lee J., Gary D.E., Wang H. Motion of flare footpoint emission and inferred electric field in reconnecting current sheets // Astrophys. J. V. 565. № 2. P. 1335−1347. 2002. https://doi.org/10.1086/324706
25. 25. Qiu J., Wang H., Cheng C.Z., Gary, D.E. Magnetic reconnection and mass acceleration in flare–coronal mass ejection events // Astrophys. J. V. 604. № 2. P. 900−905. 2004. https://doi.org/10.1086/382122
26. 26. Schou J., Scherrer P.H., Bush R.I. et al. Design and ground calibration of the Helioseismic and Magnetic Imager (HMI) instrument on the Solar Dynamics Observatory (SDO) // Solar Phys. V. 275. № 1–2. P. 229–259. 2012. https://doi.org/10.1007/s11207-011-9842-2
27. 27. Snodgrass H.B., Kress J.M., Wilson P.R. Observations of the polar magnetic fields during the polarity reversals of cycle 22 // Solar Phys. V. 191. № 1. P. 1−19. 2000. https://doi.org/10.1023/A:1005279508869
28. 28. Sterling A.C., Moore R.L. Slow-rise and fast-rise phases of an erupting solar filament, and flare emission onset // Astrophys. J. V. 630. № 2. P. 1148−1159. 2005. https://doi.org/10.1086/432044
29. 29. Sturrock P.A. Model of the high-energy phase of solar flares // Nature. V. 211. № 5050. P. 695−697. 1966. https://doi.org/10.1038/211695a0
30. 30. Švestka Z. On the varieties of solar flares / The Lower Atmosphere of Solar Flares. Proceedings of the Solar Maximum Mission Symposium. Sunspot, NM, August 20−24, 1985. Eds. Neidig D.F., Machado M.E. Sunspot, NM: National Solar Observatory. P. 332–355. 1986.
31. 31. Van Tend W., Kuperus M. The development of coronal electric current system in active regions and their relation to filaments and flares // Solar Phys. V. 59. № 1. P. 115–127. 1978. https://doi.org/10.1007/BF00154935
32. 32. Wang H., Qiu J., Jing J., Zhang H. Study of ribbon separation of a flare associated with a quiescent filament eruption // Astrophys. J. V. 593. № 1. P. 564−570. 2003. https://doi.org/10.1086/376360
33. 33. Zhang Q.M., Yang S.H., Li T., Hou Y.J., Li Y. Fast degradation of the circular flare ribbon on 2014 August 24 // Astron. Astrophys. V. 636. ID L11. 2020. https://doi.org/10.1051/0004-6361/202038072