Search for Solar Sources of Interplanetary Coronal Mass Ejections Using the Reverse Model of Magnetodynamic Interaction of the Solar Wind in the Heliosphere

Cover Page

Cite item

Full Text

Open Access Open Access
Restricted Access Access granted
Restricted Access Subscription Access

Abstract

In the development and testing of methods for predicting interplanetary coronal mass ejections (ICMEs), it is important to establish their relationship with sources on the Sun—coronal mass ejections (CMEs) observed by coronagraphs. The often used inverse ballistic calculation of the CME onset time does not consider variations in the CME speed when moving through the heliosphere and can give an uncertainty up to a day. With a good accuracy (on the order of ±10 h), the propagation of CMEs in the heliosphere from the Sun to the Earth is described by the model of the magnetodynamic interaction of CMEs with the background solar wind (drag-based model, DBM). In this paper, we propose to search for possible coronal sources of ICMEs, observed near the Earth, using the reverse model of magnetodynamic interaction (reverse DBM, RDBM), which reconstructs in the reverse course the probable propagation of CMEs in the heliosphere and determines their outflow parameters in the solar corona using the measured ICME parameters. The model uses the speed of the background solar wind, which is calculated from the area of coronal holes in the central part of the Sun and presented on the website of the Space Monitoring Data Center of the Skobeltsyn Institute of Nuclear Physics, Moscow State University (SINP MSU), with correction factors.

About the authors

D. G. Rodkin

Lebedev Physical Institute, Russian Academy of Sciences

Email: rodkindg@gmail.com
Moscow, Russia

V. A. Slemzin

Lebedev Physical Institute, Russian Academy of Sciences

Email: rodkindg@gmail.com
Moscow, Russia

Yu. S. Shugay

Skobeltsyn Institute of Nuclear Physics, Moscow State University

Author for correspondence.
Email: rodkindg@gmail.com
Moscow, Russia

References

  1. I. G. Richardson and H. V. Cane, J. Geophys. Res. 109, A09104 (2004).
  2. Ю. И. Ермолаев, Н. С. Николаева, И. Г. Лодкина, М. Ю. Ермолаев, Космич. исслед. 47, 99–113 (2009).
  3. I. G. Richardson and H. V. Cane, Solar Phys. 264, 189–237 (2010).
  4. H. S. Hudson and E. W. Cliver, J. Geophys. Res. 106, 25199 (2001).
  5. В. А. Слемзин, Ю. С. Шугай, Космич. исслед. 53, 51 (2015).
  6. R. A. Harrison, P. Bryans, G. M. Simnett, and M. Lyons, Astron. and Astrophys. 400, 1071–1083 (2003).
  7. K. Dissauer, A. M. Veronig, M. Temmer, and T. Podladchikova, Astrophys. J. 874, 123 (2019).
  8. D. M. Rust and E. Hildner, Solar Phys. 48, 381–387 (1976).
  9. H. S. Hudson, J. R. Lemen, O. C. St. Cyr, A. C. Sterling, and D. F. Webb, Geophys. Res. Lett. 25, 2481–2484 (1998).
  10. B. Vršnak, Solar Phys. 202, 173 (2001).
  11. B. Vršnak and N. Gopalswamy, J. Geophys. Res.: Space Phys. 107, 1019 (2002).
  12. P. J. Cargill, Solar Phys. 221, 135 (2004).
  13. B. Vršnak and T. Žic, Astron. and Astrophys. 472, 937 (2007).
  14. B. Vršnak, T. Žic, D. Vrbanec, M. Temmer, T. Rollett, C. Möstl, A. Veronig, J. Calogovic, M. Dumbovic, S. Lulic, Y.-J. Moon, and A. Shanmugaraju, Solar Phys. 285, 295 (2013).
  15. B. Vršnak, J. Space Weather Space Clim. 11, 34 (2021).
  16. M. Dumbovic, J. Calogovic, K. Martinic, B. Vrsnak, D. Sudar, M. Temmer, and A. Veronig, Frontiers in Astronomy and Space Sciences 8, 58 (2021).
  17. B. Vršnak, D. Ruždjak, D. Sudar, and N. Gopalswamy, Astron. and Astrophys. 423, 717–728 (2004).
  18. A. Vourlidas, S. Patsourakos, and N. P. Savani, Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 377, 20180096 (2019).
  19. Y. Shugay, V. Kalegaev, K. Kaportseva, V. Slemzin, D. Rodkin, and V. Eremeev, Universe 8, 565 (2022).
  20. G. E. Brueckner, R. A. Howard, M. J. Koomen, C. M. Korendyke, D. J. Michels, J. D. Moses, D. G. So-cker, K. P. Dere, P. L. Lamy, A. Llebaria, M. V. Bout, R. Schwenn, G. M. Simnett, D. K. Bedford, and C. J. Eyles, Solar Phys. 162, 357–402 (1995).
  21. E. Robbrecht and D. Berghmans, Astron. and Astrophys. 425, 1097–1106 (2004).
  22. E. Kraaikamp and C. J. Verbeeck, Space Weather Space Clim. 5, A18 (2015).
  23. Ю. С. Шугай, И. С. Веселовский, Д. Б. Ситон, Д. Берг-манс, Астрон. вестник 45, 560–571 (2011).
  24. S. J. Hofmeister, A. Veronig, M. Temmer, S. Vennerstrom, B. Heber, and B. Vršnak, J. Geophys. Res.: Space Phys. 123, 1738–1753 (2018).
  25. Ю. С. Шугай, Метеорология и гидрология 3, 58–66 (2021).
  26. Ю. С. Шугай, К. Б. Капорцева, Геомагнетизм и аэрономия 61, 148–159 (2021).
  27. J. Čalogović, M. Dumbović, D. Sudar, B. Vršnak, K. Mar-tinić, M. Temmer, and A. Veronig, Solar Phys. 296, 114 (2021).

Supplementary files

Supplementary Files
Action
1. JATS XML
2.

Download (128KB)

Copyright (c) 2023 Д.Г. Родькин, В.А. Слемзин, Ю.С. Шугай

This website uses cookies

You consent to our cookies if you continue to use our website.

About Cookies