Coronal dimming parameters and their variations in the 24th solar cycle

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We analyzed coronal dimming parameters and their relation to coronal mass ejections to determine the location of possible ejections sources on the solar disk in the 24th solar cycle. We used Solar Demon database that contains flares and dimmings parameters obtained from SDO/AIA image. Coronal mass ejections from the CACTus database were associated with 16% of all the dimmings for the period 2010–2018. On average, dimmings associated with coronal mass ejections are events with large absolute parameter values. Correlation coefficient between dimming position angle and associated coronal mass ejection position angle is 0.96. Correlation coefficients between the coronal mass ejection speed and dimming parameters are close to 0.5 for dimmings in the central region of the solar disk. Obtained results can be used to model coronal mass ejections propagation and to define the probability of their arrival in near-Earth space.

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作者简介

A. Vakhrusheva

Lomonosov Moscow State University (MSU)

编辑信件的主要联系方式.
Email: vakhr.anna@gmail.com

Skobeltsyn Institute of Nuclear Physics (SINP), Faculty of Physics

俄罗斯联邦, Moscow

Yu. Shugay

Lomonosov Moscow State University (MSU)

Email: vakhr.anna@gmail.com

Skobeltsyn Institute of Nuclear Physics (SINP)

俄罗斯联邦, Moscow

K. Kaportseva

Lomonosov Moscow State University (MSU)

Email: vakhr.anna@gmail.com

Skobeltsyn Institute of Nuclear Physics (SINP), Faculty of Physics

俄罗斯联邦, Moscow

V. Eremeev

Lomonosov Moscow State University (MSU)

Email: vakhr.anna@gmail.com

Skobeltsyn Institute of Nuclear Physics (SINP)

俄罗斯联邦, Moscow

V. Kalegaev

Lomonosov Moscow State University (MSU)

Email: vakhr.anna@gmail.com

Skobeltsyn Institute of Nuclear Physics (SINP), Faculty of Physics

俄罗斯联邦, Moscow

参考

  1. Черток И.М., Гречнев В.В. Крупномасштабные “димминги”, вызываемые корональными выбросами массы на Солнце, по данным SOHO/EIT в четырех линиях крайнего УФ-диапазона // Астрон. журн. Т. 80. № 11. C. 1013–1025. 2003.
  2. Черток И.М., Гречнев В.В. Некоторые проявления крупномасштабной активности на солнечном диске в связи с корональными выбросами массы // Солнечно-земная физика. Т. 6. С. 101—103. 2004.
  3. Chertok I.M., Grechnev V.V. Manifestations of CME-associated dimmings at four EUV wavelengths of SOHO/EIT // International Solar Cycle Studies Symposium 2003 “Solar Variability as an Input to the Earth’s Environment”, Tatranská Lomnica, Slovakia, 23–28 June 2003. Ed. A. Wilson. ESA SP-535
  4. Chertok I.M., Grechnev V.V. Large-scale activity in the Bastille Day 2000 solar event // Sol. Phys. V. 229. P. 95— 114. 2005. doi: 10.1007/s11207-005-3654-1
  5. Chikunova G., Dissauer K., Podladchikova T., Veronig A.M. Coronal dimmings associated with coronal mass ejections on the solar limb // Astrophys. J. V. 896. P. 17—33. 2020. doi: 10.3847/1538-4357/ab9105
  6. Compagnino A., Romano P., Zucarello F. A statistical study of CME properties and of the correlation between flares and CMEs over solar cycles 23 and 24 // Sol. Phys. V. 292. A5. 2017. doi: 10.1007/s11207-016-1029-4
  7. Dissauer K., Veronig A.M., Temmer M., Podladchikova T., Vanninathan K. Statistics of coronal dimmings associated with coronal mass ejections. I. Characteristic dimming properties and flare association // Astrophys. J. V. 863. P. 169–188. 2018. doi: 10.3847/1538-4357/aad3c6
  8. Dissauer K., Veronig A.M., Temmer M., Podladchikova T. Statistics of coronal dimmings associated with coronal mass ejections. II. Relationship between coronal dimmings and their associated CMEs // Astrophys. J. V. 874. P. 123— 137. 2019. doi: 10.3847/1538-4357/ab0962
  9. Gopalswamy N., Kaiser M.L., MacDowall R.J., Reiner M.J., Thompson B.J., St. Cyr O.C. Dynamical phenomena associated with a coronal mass ejection // AIP Conference Proceedings. V. 471. P. 641–644. 1999.
  10. Gopalswamy N., Yashiro S., Mäkelä P., Michalek G., Shibasaki K., Hathaway D.H. Behavior of solar cycles 23 and 24 revealed by microwave observations // Astrophys. J. Lett. V. 750. L42. 2012. doi: 10.1088/2041-8205/750/2/L42
  11. Hansen R.T., Garcia C.J., Hansen S.F., Yasukawa E. Abrupt depletions of the inner corona // Pub. Astron. Soc. Pacific. V. 86. P. 500— 515. 1974. doi: 10.1086/129638
  12. Harra L.K., Sterling A.C. Material outflows from coronal intensity “dimming regions” during coronal mass ejection onset // Astrophys. J. Lett. V. 561 L215–L218. 2001. doi: 10.1086/324767
  13. Harrison R.A., Bryans P., Simnett G.M., Lyons M. Coronal dimming and the coronal mass ejection onset // Astron. Astrophys. V. 400. P. 1071–1083. 2003. doi: 10.1051/0004-6361:20030088
  14. Hudson H.S., Acton L.W., Freeland S.L. A long-duration solar flare with mass ejection and global consequences // Astrophys. J. V. 470 P. 629–635. 1996. doi: 10.1086/177894
  15. Hudson H.S., Webb D.F. Soft X-ray signatures of coronal ejections // Geophys. Monogr. Ser. V. 99. Eds. N. Crooker, J. A. Joselyn, J. Feynman. P. 27–38. Washington, AGU. 1997. doi: 10.1029/GM099p0027
  16. Hurlburt N., Cheung M., Schrijver C., et al. Heliophysics event knowledgebase for the Solar Dynamics Observatory (SDO) and beyond // Sol. Phys. V. 275 P. 67–78. 2012. doi: 10.1007/s11207-010-9624-2
  17. Jin M., Cheung M.C.M., DeRosa M.L., Nitta N.V., Schrijver C.J. Coronal mass ejections and dimmings: a comparative study using MHD simulations and SDO observations // Astrophys. J. V. 928. № 2. P. 154–165. 2022. doi: 10.3847/1538-4357/ac589b
  18. Kraaikamp E., Verbeeck C. Solar Demon — an approach to detecting flares, dimmings and EUV waves on SDO/AIA images // J. Space Weather Spac. V. 5 A18. 2015. doi: 10.1051/swsc/2015019
  19. Lamy P.L., Floyd O., Boclet B., Wojak J., Gilardy H., Barlyaeva T. Coronal mass ejections over solar cycles 23 and 24 // Space Sci. Rev. V. 215. A39. 2019. doi: 10.1007/s11214-019-0605-y
  20. López F.M., Cremades H., Balmaceda L.A., Nuevo F.A., Vásquez A.M. Estimating the mass of CMEs from the analysis of EUV dimmings // Astron. Astrophys. V. 627 A8. 2019. doi: 10.1051/0004-6361/201834163
  21. Mason J.P., Woods T.N., Webb D.F., Thompson B.J., Colaninno R.C., Vourlidas A. Relationship of EUV irradiance coronal dimming slope and depth to coronal mass ejection speed and mass // Astrophys. J. V. 830. № 1. P. 20–31. 2016. doi: 10.3847/0004-637X/830/1/20
  22. Muhr N., Veronig A.M., Kienreich I.W., Temmer M., Vršnak B. Analysis of characteristic parameters of large-scale coronal waves by the Solar-Terrestrial Relations Observatory / Extreme Ultraviolet Imager // Astrophys. J. V. 739. № 2. A. 89. 2011. doi: 10.1088/0004-637X/739/2/89
  23. NASA Interactive Multi-Instrument Database of Solar Flares https://data.nas.nasa.gov/helio/portals/solarflares/
  24. NASA SOHO LASCO CME CATALOG — CDAW DATA CENTER. https://cdaw.gsfc.nasa.gov/CME_list/
  25. Podladchikova T., Veronig A.M., Dissauer K., Temmer M., Podladchikova O. Three-dimensional reconstructions of extreme-ultraviolet wave front heights and their influence on wave kinematics // Astrophys. J. V. 877. № 2. A. 68. 2019. doi: 10.3847/1538-4357/ab1b3a
  26. Reinard A.A., Biesecker D.A. Coronal mass ejection — associated coronal dimmings // Astrophys. J. V. 674. P. 576— 585. 2008. doi: 10.1086/525269
  27. Robbrecht E., Berghmans D., Van der Linden R.A.M. Automated LASCO CME catalog for solar cycle 23: are CMEs scale invariant? // Astrophys. J. V. 691. № 2. P. 1222–1234. 2009. doi: 10.1088/0004-637X/691/2/1222
  28. Rodkin D., Slemzin V., Zhukov A.N., Goryaev F., Shugay Y., Veselovsky I. Single ICMEs and complex transient structures in the solar wind in 2010–2011 // Sol. Phys. V. 293. A. 78. 2018. doi: 10.1007/s11207-018-1295-4
  29. Rust D.M., Hildner E. Expansion of an X-ray coronal arch into the outer corona // Sol. Phys. V. 48. P. 381–387. 1976. doi: 10.1007/BF00152003
  30. Shugai Y.S. Analysis of quasistationary solar wind stream forecasts for 2010-2019 // Russian Meteorology and Hydrology. V. 46. P. 172–178. 2021. doi: 10.3103/s1068373921030055
  31. Shugay Y., Kalegaev V., Kaportseva K., Slemzin V., Rodkin D., Eremeev V. Modeling of solar wind disturbances associated with coronal mass ejections and verification of the forecast results // Universe. V. 8. № 11. P. 565–585. 2022. doi: 10.3390/universe8110565
  32. Solar Influences Data Analysis Center (Royal Observatory of Belgium) Solar Demon — Flares, Dimmings and EUV waves event detection. https://www.sidc.be/solardemon/
  33. Solar Influences Data Analysis Center (Royal Observatory of Belgium) CACTus CME Homepage. https://www.sidc.be/cactus/
  34. Solar Influences Data Analysis Center (Royal Observatory of Belgium) Sunspot Number | SILSO https://www.sidc.be/silso/datafiles
  35. Sterling A.C., Hudson H.S. Yohkoh SXT observations of X-ray “dimming” associated with a halo coronal mass ejection // Astrophys. J. V. 491. № 1. P. L55–L58. 1997. doi: 10.1086/311043
  36. Ternullo M. Looking inside the butterfly diagram // Astronomische Nachrichten. V. 328. № 10. P. 1023–1026. 2007. doi: 10.1002/asna.200710868
  37. Vanninathan K., Veronig A.M., Dissauer K., Temmer M. Plasma diagnostics of coronal dimming events // Astrophys. J. V. 857. P. 62–83. 2018. doi: 10.3847/1538-4357/aab09a
  38. Veronig A.M., Podladchikova T., Dissauer K., Temmer M., Seaton D.B., Long D., Guo J., Vršnak B., Harra L., Kliem B. Genesis and impulsive evolution of the 2017 September 10 coronal mass ejection // Astrophys. J. V. 868. № 2. A. 107. 2018. doi: 10.3847/1538-4357/aaeac5
  39. Webb D.F., Lepping R.P., Burlaga L.F., DeForest C.E., Larson D.E., Martin S.F., Plunkett S.P., Rust D.M. The origin and development of the May 1997 magnetic cloud // J. Geophys. Res. V. 105. № A12. P. 27251— 27260. 2000. doi: 10.1029/2000JA000021
  40. Xie H., Ofman L., Lawrence G. Cone model for halo CMEs: application to space weather forecasting // J. Geophys. Res. V. 109. A03109. 2004. doi: 10.1029/2003JA010226
  41. Yashiro S., Michalek G., Gopalswamy N. A comparison of coronal mass ejections identified by manual and automatic methods // Ann. Geophysicae. V. 26. № 10. P. 3103— 3112. 2008. doi: 10.5194/angeo-26-3103-2008

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2. Fig. 1. Calculation of the position angle for dimming (left) and VCR (right).

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3. Fig. 2. Histograms of the distribution of dimming parameters: (a) – maximum value of the full brightness module; (b) — maximum brightness jump; (c) — maximum area; (d) — dimming duration. On the Y axis on the left is the number of events for all dimmings (black columns), on the right is the number of events for dimmings associated with the CME (shaded columns). The curves indicate the density approximation of the lognormal distribution.

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4. Fig. 3. Variations in solar activity events over the years. On the Y axis on the left is the number of events (dimmings, flares, CMEs), on the right is the annual average number of sunspots according to WDC-SILSO data (https://www.sidc.be/silso/datafiles).

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5. Fig. 4. Dependence of the average dimming latitude on time for 2010–2018.

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6. Fig. 5. Dependence of the average CME speed in the coronagraph on the maximum dimming area for all corresponding CMEs and dimmings. The straight line denotes the linear dependence of the logarithms of the parameters.

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7. Fig. 6. Dependence of the average CME speed in the coronagraph on the maximum dimming area. The calculation was made for a sample of dimmings from the central region of the solar disk. The straight line denotes the linear dependence of the logarithms of the parameters.

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8. Fig. 7. Dependence of the VCR position angle on the dimming position angle. The straight line denotes the linear dependence of the parameters.

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