Laboratory Modelling of Solar Wind Interaction with Lunar Magnetic Anomalies

Capa

Citar

Texto integral

Acesso aberto Acesso aberto
Acesso é fechado Acesso está concedido
Acesso é fechado Somente assinantes

Resumo

The paper presents the results of laboratory experiment modeling the interaction between Lunar magnetic anomalies and Solar wind. To model the LMA we use quadrupole magnetic field. The main dimensionless parameter of the problem, the ion inertia length relative to the mini-magnetosphere size, well corresponds between experiment and LMA conditions. The main result is measurement of the magnetically reflected proton fluxes, which show qualitative agreement to available satellite data.

Sobre autores

M. Rumenskikh

Laser Physics Department, Institute of Laser Physics; Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia; Moscow, Russia

A. Chibranov

Laser Physics Department, Institute of Laser Physics

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

M. Efimov

Laser Physics Department, Institute of Laser Physics

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

A. Berezutsky

Laser Physics Department, Institute of Laser Physics

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

V. Posukh

Laser Physics Department, Institute of Laser Physics

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

P. Trushin

Laser Physics Department, Institute of Laser Physics

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

Yu. Zakharov

Laser Physics Department, Institute of Laser Physics

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

E. Boyarintsev

Laser Physics Department, Institute of Laser Physics

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

I. Miroshnichenko

Laser Physics Department, Institute of Laser Physics

Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

A. Divin

Physics Department, St. Petersburg State University

Email: marina_rumenskikh@mail.ru
St. Petersburg, Russia

I. Shaikhislamov

Laser Physics Department, Institute of Laser Physics

Autor responsável pela correspondência
Email: marina_rumenskikh@mail.ru
Novosibirsk, Russia

Bibliografia

  1. M. Wieser, S. Barabash, Y. Futaana, Geophys. Res. Lett. 37 (2010).
  2. C. Richmond, L. L. Hood, J. Geophys. Res. vol. 113 (2008).
  3. J. S. Halekas, D. L. Mitchell, R. P. Lin, S. Frey, L. L. Hood, M. H. Acuna, A. B. Binder, J. Geophys. Res. 106, 27841–27852.
  4. H. Tsunakawa, F. Takahashi, H. Shimizu, H. Shibuya, M. Matsushima, J. Geophys. Res. Planets, 120, 1160–1185 (2015).
  5. J. S. Halekas, G. T. Delory, D. A. Brain, R. P. Lin, D. L. Mitchell, Plan. and Space Sci. 56, 941–946 (2008).
  6. R. P. Lin, D. L. Mitchell, D. W. Curtis, et al., Science 281, 1480 (1998).
  7. А. А. Скальский, А. М. Садовский, Космические исследования, т. 53, № 1, 75–78 (2015).
  8. Y. Saito, S. Yokota, T. Tanaka, et al., Geophys. Res. Lett. 35, L24205 (2008).
  9. Y. Saito, M. N. Nishino, M. Fujimoto, et al., Earth Planets Space. 64, 83 (2012).
  10. M. Wieser, S. Barabash, Y. Futaana, et al., Plan. and Space Sci. 57, 2132 (2009).
  11. M. Holmström, M. Wieser, S. Barabash, et al., J. Geophys. Res. 115, A06206 (2010).
  12. L. L. Hood, G. Schubert, Science 208, № 4439, 49–51 (1980).
  13. D. T. Blewett, et al., J. Geophys. Res.: Planets 116, № E2 (2011).
  14. I. Garrick-Bethell, J. W. Head III, C. M. Pieters, Icarus 212, № 2, 480–492 (2011).
  15. J. Deca, et al., J. Geophys. Res.: Planets 125, № 5 (2020).
  16. B. W. Denevi, et al., Icarus 273, 53–67 (2016).
  17. D. Hemingway, I. Garrick-Bethell, J. Geophys. Res.: Planets 117, № E10 (2012).
  18. J. Gattacceca, et al., Earth and Planetary Science Letters 299, № 1–2, 42–53 (2010).
  19. E. Kallio, R. Jarvinen, S. Dyadechkin, P. Wurz, S. Ba-rabash, Geophys. Res. Abstracts 14, EGU 2012–4937 (2012).
  20. J. Deca, A. Divin, G. Lapenta, Phys. Rev. Lett. 112, 151102 (2014).
  21. J. Deca, et al. J. Geophys. Res. Space Physics 120.8, 6443–6463 (2015).
  22. R. A. Bamford, B. Kellett, W. J. Bradford, C. Norberg, A. Thornton, K. J. Gibson, R. Bingham, Phys. Rev. Lett. 109 (8), 081101 (2012).
  23. J. Han, Laboratory simulation of solar wind interaction with a magnetic dipole field on lunar surface: диc. – University of Colorado, 2017.
  24. I. F. Shaikhislamov, V. M. Antonov, Y. P. Zakharov, E. L. Boyarintsev, A. V. Melekhov, V. G. Posukh, A. G. Po-nomarenko, Advances in Space Research 52 (3), 422–436 (2013).
  25. I. F. Shaikhislamov, Y. P. Zakharov, V. G. Posukh, A. V. Me-lekhov, V. M. Antonov, E. L. Boyarintsev, A. G. Ponomarenko, Plasma Physics and Controlled Fusion 56 (2), 025004 (2014).
  26. I. F. Shaikhislamov, V. G. Posukh, A. V. Melekhov, Y. P. Za-kharov, E. L. Boyarintsev, A. G. Ponomarenko, Plasma Physics and Controlled Fusion 57 (7), 075007 (2015).
  27. I. F. Shaikhislamov, Y. P. Zakharov, V. G., Posukh, A. V. Melekhov, E. L. Boyarintsev, A. G. Ponomarenko, V. A. Terekhin, Plasma Physics Reports 41 (5), 399–407 (2015).
  28. K. J. Fujita, Space Technol. Sci. 20 (2), 26–31 (2004).
  29. N. Omidi, X. Blanco-Cano, C. T. Russell, H. Karimabadi, M. Acuna, J. Geophys. Res. 107 (A12), 1487 (2002).
  30. M. Kurata, H. Tsunakawa, Y. Saito, H. Shibuya, M. Matsushima, H. Shimizu, Geophys. Res. Lett. 32 (24) (2005).
  31. M. E. Purucker, J. B. Nicholas, J. Geophys. Res.: Planets 115, E12 (2010).
  32. D. Ravat, M. E. Purucker, N. Olsen, J. Geophys. Res.: Planets 125 (7), e2019JE006187 (2020).
  33. M.S. Rumenskikh, A. A., Chibranov, M.A. Efimov, JETPh Letters 111 (6), 335 (2020).
  34. Q. Wang, J. Cui, D. Wang, Advances in Space Research 50 (12), 1600 (2012).
  35. C. Lue, Y. Futaana, S. Barabash, M. Wieser, M. Holmström, A. Bhardwaj, … P. Wurz, Geophys. Res. Lett. 38 (3) (2011).

Arquivos suplementares

Arquivos suplementares
Ação
1. JATS XML
2.

Baixar (309KB)
3.

Baixar (111KB)
4.

Baixar (122KB)
5.

Baixar (45KB)
6.

Baixar (194KB)
7.

Baixar (46KB)

Declaração de direitos autorais © М.С. Руменских, А.А. Чибранов, М.А. Ефимов, А.Г. Березуцкий, В.Г. Посух, П.А. Трушин, Ю.П. Захаров, Э.Л. Бояринцев, И.Б. Мирошниченко, А.В. Дивин, И.Ф. Шайхисламов, 2023

Este site utiliza cookies

Ao continuar usando nosso site, você concorda com o procedimento de cookies que mantêm o site funcionando normalmente.

Informação sobre cookies