1960
DOI: 10.1103/revmodphys.32.951
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Shock Waves and Shock-Wave Structure in Magneto-Fluid Dynamics

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Cited by 102 publications
(37 citation statements)
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“…It has been suggested by [9] Germain that, to some degree, there appears to have been two avenues of shock wave studies.…”
Section: Introductionmentioning
confidence: 99%
“…It has been suggested by [9] Germain that, to some degree, there appears to have been two avenues of shock wave studies.…”
Section: Introductionmentioning
confidence: 99%
“…Germain 1960;Anderson 1963;Jeffrey and Taniuti 1964;Liberman and Velikhovich 1986;Sturtevant 1987;Gombosi 1998;Goedbloed 2008) and just express the basic nonlinear conservation laws across a discontinuity. Discontinuous solutions only satisfy the integral form of the MHD equations, i.e.…”
Section: Intermediate Shocks In Mhdmentioning
confidence: 99%
“…For dissipative models in simple geometries in the limit of vanishing dissipation, the intermediate shocks were shown not to be stable against certain perturbations. Traditionally ͑Akhiezer, Liubarski, and Polovin, 9 Germain, 10 Jeffrey and Taniuti 11 ͒, this failure of the test of evolutionarity was used to rule out the physical reality of intermediate shocks. However, after Wu 13 showed intermediate shocks to arise in numerical solutions of the dissipative MHD equations, a flurry of numerical and observational papers appeared on the structure and formation of intermediate shocks, [25][26][27][28][29] on their astrophysical implications, 30,31 on their relationship with magnetic reconnection, 32,33 on their significance for the Riemann problem, [34][35][36] on their occurrence in bow-shock flows, 37 and their possible breakup.…”
Section: -17mentioning
confidence: 99%
“…7,8 In the theory of shock conditions in magnetohydrodynamics ͑MHD͒, the so-called intermediate shocks play a prominent role since they continuously connect the slow and fast magnetosonic shocks in parameter space. In the older literature, [9][10][11][12] these shocks were discarded because they were believed to be nonevolutionary. However, in 1988, Wu 13 showed intermediate shocks to arise in a numerical solution of the dissipative MHD equations through nonlinear steepening from a continuous wave.…”
Section: Introductionmentioning
confidence: 99%