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

A. A. Vakhrusheva; Вахрушева А. А.; Yu. S. Shugay; Шугай Ю. С.; K. B. Kaportseva; Капорцева К. Б.; V. E. Eremeev; Еремеев В. Е.; V. V. Kalegaev; Калегаев В. В.

doi:10.31857/S0016794024010017

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

Авторлар: Vakhrusheva A.A.¹, Shugay Y.S.¹, Kaportseva K.B.¹, Eremeev V.E.¹, Kalegaev V.V.¹
Мекемелер:
1. Lomonosov Moscow State University (MSU)
Шығарылым: Том 64, № 1 (2024)
Беттер: 3-12
Бөлім: Articles
URL: https://journal-vniispk.ru/0016-7940/article/view/260737
DOI: https://doi.org/10.31857/S0016794024010017
EDN: https://elibrary.ru/GRSFFB
ID: 260737

Дәйексөз келтіру

Толық мәтін

Ашық рұқсат
Рұқсат жабық

Рұқсат берілді
Рұқсат жабық

Тек жазылушылар үшін

Аннотация
Толық мәтін
Авторлар туралы
Әдебиет тізімі
Қосымша файлдар
Статистика

Аннотация

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.

Толық мәтін

Ресей, Moscow

Әдебиет тізімі

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.
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.
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
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
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
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
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
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
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.
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
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
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
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
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
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
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
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
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
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
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
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
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
NASA Interactive Multi-Instrument Database of Solar Flares https://data.nas.nasa.gov/helio/portals/solarflares/
NASA SOHO LASCO CME CATALOG — CDAW DATA CENTER. https://cdaw.gsfc.nasa.gov/CME_list/
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
Reinard A.A., Biesecker D.A. Coronal mass ejection — associated coronal dimmings // Astrophys. J. V. 674. P. 576— 585. 2008. doi: 10.1086/525269
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
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
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
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
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
Solar Influences Data Analysis Center (Royal Observatory of Belgium) Solar Demon — Flares, Dimmings and EUV waves event detection. https://www.sidc.be/solardemon/
Solar Influences Data Analysis Center (Royal Observatory of Belgium) CACTus CME Homepage. https://www.sidc.be/cactus/
Solar Influences Data Analysis Center (Royal Observatory of Belgium) Sunspot Number | SILSO https://www.sidc.be/silso/datafiles
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
Ternullo M. Looking inside the butterfly diagram // Astronomische Nachrichten. V. 328. № 10. P. 1023–1026. 2007. doi: 10.1002/asna.200710868
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
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
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
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
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

Қосымша файлдар

Әрекет

1. JATS XML

Жүктеу

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

Жүктеу (172KB)

Метадеректер

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.

Жүктеу (577KB)

Метадеректер

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).

Жүктеу (180KB)

Метадеректер

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

Жүктеу (132KB)

Метадеректер

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.

Жүктеу (103KB)

Метадеректер

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.