Observation of mirror waves downstream of a quasi-perpendicular shock
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C. Perche | Christopher T. Russell | D. Hubert | C. Russell | Daan Hubert | Christopher C. Harvey | C. Lacombe | C. Lacombe | C. Harvey | C. Perche
[1] Charles C. Goodrich,et al. The structure of perpendicular bow shocks , 1982 .
[2] P. Kellogg,et al. Electrostatic noise at the plasma frequency beyond the earth's bow shock , 1979 .
[3] P. Rodriguez. Long duration lion roars associated with quasi‐perpendicular bow shocks , 1985 .
[4] C. Russell,et al. The ISEE 1 and 2 Fluxgate Magnetometers , 1978, IEEE Transactions on Geoscience Electronics.
[5] C. Russell,et al. Evolution of ion distributions across the nearly perpendicular bow shock: Specularly and non‐specularly reflected‐gyrating ions , 1983 .
[6] J. King. Interplanetary medium data book , 1977 .
[7] C. Kennel,et al. A parametric survey of the first critical Mach number for a fast MHD shock , 1984, Journal of Plasma Physics.
[8] D. Winske,et al. Magnetic field and density fluctuations at perpendicular supercritical collisionless shocks , 1988 .
[9] B. Tsurutani,et al. The generation mechanism for magnetosheath lion roars , 1981, Nature.
[10] D. Baker,et al. Lion roars and nonoscillatory drift mirror waves in the magnetosheath , 1982 .
[11] Lou‐Chuang Lee,et al. A study of mirror waves generated downstream of a quasi‐perpendicular shock , 1988 .
[12] D. Fairfield. Magnetic fields of the magnetosheath , 1976 .
[13] A. Wolfe,et al. Large‐amplitude hydromagnetic waves in the inner magnetosheath , 1970 .
[14] C. Russell,et al. The resolved layer of a collisionless, high β, supercritical, quasi‐perpendicular shock wave: 1. Rankine‐Hugoniot geometry, currents, and stationarity , 1986 .
[15] Daniel W. Swift,et al. Numerical simulation of nonoscillatory mirror waves at the Earth's magnetosheath , 1986 .