Zakharov–Kuznetsov Equation for Describing Low-Frequency Nonlinear Dust Acoustic Perturbations in Saturn’s Dusty Magnetosphere

Capa

Citar

Texto integral

Resumo

A description is given of low-frequency nonlinear dust acoustic waves in Saturn’s dusty magnetosphere, which contains electrons of two types (hot and cold) obeying the kappa distribution, magnetospheric ions, and charged dust particles. For the corresponding conditions, the derivation of the Zakharov–Kuznetsov equation is given, which describes the nonlinear dynamics of dust acoustic waves in the case of low frequencies and a pancake-shaped wave packet along an external magnetic field. It is shown that under the conditions of Saturn’s magnetosphere there exist solutions of the Zakharov–Kuznetsov equation in the form of one-dimensional and three-dimensional solitons. Possible observations of the considered solitons in future space missions are discussed.

Texto integral

Acesso é fechado

Sobre autores

S. Kopnin

Space Research Institute, Russian Academy of Sciences

Email: popel@iki.rssi.ru
Rússia, Moscow

D. Shokhrin

Higher School of Economics

Email: popel@iki.rssi.ru
Rússia, Moscow

S. Popel

Space Research Institute, Russian Academy of Sciences

Autor responsável pela correspondência
Email: popel@iki.rssi.ru
Rússia, Moscow

Bibliografia

  1. Попель С.И. // Природа. 2015. № 9. С. 48.
  2. Wahlund J.-E., André M., Eriksson A.I.E., Lundberg M., Morooka M.W., Shafiq M., Averkamp T.F., Gurnett D.A., Hospodarsky G.B., Kurth W.S., Jacobsen K.S., Pedersen A., Farrell W., Ratynskaia S., Piskunov N. // Planetary Space Sci. 2009. V. 57. P. 1795.
  3. Yaroshenko V.V., Ratynskaia S., Olson J., Brenning N., Wahlund J.-E., Morooka M., Kurth W.S., Gurnett D.A., Morfill G.E. // Planetary Space Sci. 2009. V. 57. P. 1807.
  4. Sittler Jr. E.C., Ogilvie K.W., Scudde J.D. // J. Geophys. Res. 1983. V. 88. P. 8847.
  5. Barbosa D.D., Kurth W.S. // J. Geophys. Res. 1993. V. 98. P. 9351.
  6. Koen E.J., Collier A.B., Maharaj S.K., Hellberg M.A. // Phys. Plasmas. 2014. V. 21. P. 072122.
  7. Popel S.I., Zelenyi L.M., Golub’ A.P., Dubinskii A.Yu. // Planetary Space Sci. 2018. V. 156. P. 71.
  8. Голубь А.П., Попель С.И. // Письма ЖЭТФ. 2021.Т. 113. С. 440.
  9. Schippers P., Blanc M., Andre N., Dandouras I., Lewis G.R., Gilbert L.K., Persoon A.M., Krupp N., Gurnett D.A., Coates A.J., Krimigis S.M., Young D.T., Dougherty M.K. // J. Geophys. Res. 2008. V. 113. P. A07208.
  10. Yeager A. // Nature. 2008. doi: 10.1038/news.2008.1254.
  11. Pécseli H.L., Lybekk B., Trulsen J., Eriksson A. // Plasma Phys. Controlled Fusion. 1997. V. 39. P. A227.
  12. Попель С.И. // Физика плазмы. 2001. Т. 27. С. 475.
  13. Копнин С.И., Косарев И.Н., Попель С.И. // Физика плазмы. 2005. Т. 31. С. 224.
  14. Копнин С.И., Шохрин Д.В., Попель С.И. // Физика плазмы. 2022. Т. 48. С. 163.
  15. Копнин С.И., Шохрин Д.В., Попель С.И. // Физика плазмы. 2023. Т. 49. С. 582.
  16. Петвиашвили В.И., Похотелов О.А. Уединенные волны в плазме и атмосфере. М.: Энергоатомиздат, 1989.
  17. Banerjee G., Maitra S. // Phys. Plasmas. 2015. V. 22. P. 043708.
  18. Popel S.I., Kopnin S.I., Kosarev I.N., Yu M.Y. // Adv. Space Res. 2006. V. 37. P. 414.
  19. Rubab N., Murtaza G. // Physica Scripta. 2006. V. 73. P. 178.
  20. Зейтунян Р.Х. // УФН. 1995. Т. 165. С. 1403.
  21. Рыскин Н.М., Трубецков Д.И. Нелинейные волны. М.: URSS, 2021. С. 180.
  22. Кассем А.И., Копнин С.И., Попель С.И., Зеленый Л.М. // Физика плазмы. 2022. T. 48. P. 871.
  23. Sulaiman A.H., Kurth W.S., Hospodarsky G.B., Averkamp T.F., Ye S.-Y., Menietti J.D., Farrell W.M., Gurnett D.A., Persoon A.M., Dougherty M.K., Hunt G.J. // Geophys. Res. Lett. 2018. V. 45. P. 7347.
  24. Kopnin S.I., Kosarev I.N., Popel S.I., Yu M.Y. // Planetary Space Sci. 2004. V. 52. P. 1187.

Arquivos suplementares

Arquivos suplementares
Ação
1. JATS XML
Baixar
2. Fig. 1. Characteristic view of one-dimensional solitons propagating at the angle J to the magnetic field: J = 1° - solid curve, J = 3° - dashed curve, J = 5° - dashed curve. The graphs are plotted for three cases of possible dust particle concentrations: nd0 = 10-4 cm-3 (a), nd0 = 10-3 cm-3 (b), nd0 = 10-2 cm-3 (c)

Baixar (138KB)
Metadados
3. Fig. 2. Moduli of the amplitudes of the soliton solutions (67) as a function of the characteristic mean dust particle sizes a and the soliton propagation velocity u at J = 5° for nd0 = 10-4 cm-3 (a), nd0 = 10-3 cm-3 (b), nd0 = 10-2 cm-3 (c)

Baixar (145KB)
Metadados
4. Fig. 3. Three-dimensional soliton for the cases: nd0 = 10-2 cm-3 (a), nd0 = 10-3 cm-3 (b), nd0 = 10-4 cm-3 (c)

Baixar (194KB)
Metadados

Declaração de direitos autorais © Russian Academy of Sciences, 2024