Abstract
Effect of turbulence on interplanetary shock waves propagation is considered. It is shown that background turbulence results in the additional shock wave deceleration which may be comparable with the deceleration due to plasma sweeping. The turbulent deceleration is connected with the energy losses due to the strong turbulence amplification behind the moving shock front.
Similar content being viewed by others
References
Blokhintsev, D.I.: 1981,Acoustics of inhomogeneous moving medium.Nauka.Moscow.1, 1.
Dryer, M.: 1974,Space Sci. Rev. 15, 403.
Dryer, M., Wu, S.T., Gislason, G., et al.: 1984,Astrophys. Space Sci. 105, 187.
Jascues, S.A.: 1977,Astrophys. J. 215, 942.
Landau, L.D., and Lifshits, E.M.: 1986,Hydrodynamics.Nauka.Moscow.1, 1.
Parker, E.N.: 1961,Astrophys. J. 133, 1014.
Vlasov, V.I.: 1988,Geomagnetizm i aeronomie. 28, 1.
Watanabe, T., and Kakinuma, T.: 1984,Adv. Space Res. 4, 331.
Watanabe, T., and Schwenn, R.: 1989,Space Sci. Rev. 51, 147.
Woo, R., Armstrong, J.W., Sheely, N.R., et al.: 1985,Nature. 90, 154.
Woo, R., and Schwenn, R.: 1991,Geophys. Res. 96, 21 227.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Chashei, I.V., Shishov, V.I. Shock waves propagation in the turbulent interplanetary plasma. Astrophys Space Sci 243, 23–28 (1996). https://doi.org/10.1007/BF00644028
Issue Date:
DOI: https://doi.org/10.1007/BF00644028