On the Formation of Clouds in the Dusty Ionosphere of Mars

Capa

Citar

Texto integral

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

Resumo

Dusty plasma clouds observed at altitudes of about 100 km in the mesosphere of Mars have been considered. Features of the dusty ionosphere of Mars compared to the dusty ionosphere of the Earth have been listed. The equations of the model describing self-consistently dusty plasma structures in the ionosphere of Mars have been presented. This model involves features that are important for the ionosphere of Mars but are ignored when describing the dusty plasma system in the ionosphere of the Earth. In particular, the model for Mars involves effects of deceleration of dust particles because of the adhesion of condensed molecules to them. An altitude distribution of particles constituting mesospheric clouds on Mars has been calculated with the self-consistent model. It has been shown that an important factor for the formation of dusty plasma clouds in the ionosphere of Mars is the Rayleigh–Taylor instability, which limits both the maximum size of dust particles that can form dusty plasma clouds and the maximum thickness of the dusty plasma clouds.

Sobre autores

Yu. Reznichenko

Moscow Institute of Physics and Technology (National Research University)

Email: popel@iki.rssi.ru
141700, Dolgoprudnyi, Moscow region, Russia

A. Dubinskiy

Space Research Institute, Russian Academy of Sciences

Email: popel@iki.rssi.ru
117997, Moscow, Russia

S. Popel'

Space Research Institute, Russian Academy of Sciences; National Research University Higher School of Economics

Autor responsável pela correspondência
Email: popel@iki.rssi.ru
117997, Moscow, Russia; 101000, Moscow, Russia

Bibliografia

  1. F. Montmessin, J.-L. Bertaux, E. Qu'emerais, O. Korablev, P. Rannou, F. Forget, S. Perrier, D. Fussen, S. Lebonnois, A. R'eb'erac, E. Dimarellis, Icarus 183, 403 (2006).
  2. https://www.newsru.com/hitech/30may2021/mars_clouds.html.
  3. U. von Zahn, G. Baumgarten, U. Berger, J. Fiedler, and P. Hartogh, Atmos. Chem. Phys. 4, 2449 (2004).
  4. Б. А. Клумов, Г. Е. Морфилл, С. И. Попель, ЖЭТФ 127, 171 (2005).
  5. А. Ю. Дубинский, Ю. С. Резниченко, С. И. Попель, Физика плазмы 45, 913 (2019).
  6. Yu. S. Reznichenko, A. Yu. Dubinskii, and S. I. Popel, J. Phys.: Conf. Ser. 1556, 012072 (2020).
  7. В. Н. Цытович, УФН 167, 57 (1997).
  8. В. Е. Фортов, А. Г. Храпак, С. А. Храпак, В. И. Молотков, О. Ф. Петров, УФН 174, 495 (2004).
  9. V. N. Tsytovich, G. E. Mor ll, S. V. Vladimirov, and H. M. Thomas, Elementary Physics of Complex Plasmas, Springer, Berlin (2008).
  10. В. Е. Фортов, Ю. М. Батурин, Г. О. Морфилл, О. Ф. Петров, Плазменный кристалл, Космические эксперименты, М.: Физматлит (2015).
  11. А. Ю. Дубинский, С. И. Попель, Письма в ЖЭТФ 96, 22 (2012).
  12. F. Forget, F. Montmessin, J. L. Bertaux, F. Gonzalez-Galindo, S. Lebonnois, E. Qu'emerais, A. R'eb'erac, E. Dimarellis, and M. A. Lopez-Valverde, J. Geophys. Res. 114, E01004 (2009).
  13. J. L. Fox, M. Benna, P. R. Maha y, B. M. Jakosky, Geophys. Res. Lett. 42, 8977 (2015).
  14. J.-L. Bertaux, O. Korablev, S. Perrier, E. Qu'emerais, F. Montmessin, F. Leblanc, S. Lebonnois, P. Rannou, F. Lef'evre, F. Forget, A. Fedorova, E. Dimarellis, A. Reberac, D. Fonteyn, J. Y. Chaufray, and S. Guibert, J. Geophys. Res. 111, E10S90 (2006).
  15. J.-L. Bertaux, D. Fonteyn, O. Korablev et al. (Collaboration), Eur. Space Agency Spec. Publ., ESA-SP 1240, 95 (2004).
  16. M. J. Campbell, J. Liesegang, J. D. Riley, and J. G. Jenkin, J. Phys. C: Solid State Phys. 15, 2549 (1982).
  17. М. А. Леонтович, Введение в термодинамику, Гос. изд-во технико-теоретической литературы, М., Л. (1952), c. 158.
  18. B. A. Klumov, S. I. Popel, and R. Bingham, Письма в ЖЭТФ 72, 524 (2000).
  19. F. F. Chen, in Plasma Diagnostic Techniques, ed. by R. H. Huddlestone and S. L. Leonard, Academic, N.Y. (1965), ch. 4.
  20. M. S. Barnes, J. H. Keller, J. C. Forster, J. A. O'Neill, and D. K. Coultas, Phys. Rev. Lett. 68, 313 (1992).
  21. C. V¨oltz, W. Pesch, and I. Rehberg, Phys. Rev. E. 65, 011404 (2001).
  22. Р. С. Савельев, Н. Н. Розанов, Г. Б. Сочилин, С. А. Чивилихин, Научно-технический вестник Санкт-Петербургского государственного университета информационных технологий, механики и оптики 3(73), 18 (2011).

Arquivos suplementares

Arquivos suplementares
Ação
1. JATS XML

Declaração de direitos autorais © Российская академия наук, 2023