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Shocks and discontinuities (magnetohydrodynamics)Shocks and discontinuities are transition layers where the plasma properties change from one equilibrium state to another. The relation between the plasma properties on both sides of a shock or a discontinuity can be obtained from the conservative form of the magnetohydrodynamic (MHD) equations, assuming conservation of mass, momentum, energy and of . Additional recommended knowledge
RankineHugoniot jump conditions for MHDThe jump conditions across a MHD shock or discontinuity are referred as the RankineHugoniot equations for MHD. In the frame moving with the shock/discontinuity, those jump conditions can be written:
where ρ, v, p, B are the plasma density, velocity, (thermal) pressure and magnetic field respectively. The subscripts t and n refer to the tangential and normal components of a vector (with respect to the shock/discontinuity front). The subscripts 1 and 2 refer to the two states of the plasma on each side of the shock/discontinuity Contact and tangential discontinuitiesContact and tangential discontinuities are transition layers across which there is no particle transport. Thus, in the frame moving with the discontinuity, v_{n1} = v_{n2} = 0. Contact discontinuities are discontinuities for which the thermal pressure, the magnetic field and the velocity are continuous. Only the mass density and temperature change. Tangential discontinuities are discontinuities for which the total pressure (sum of the thermal and magnetic pressures) is conserved. The normal component of the magnetic field is identically zero. The density, thermal pressure and tangential component of the magnetic field vector can be discontinuous across the layer. ShocksShocks are transition layers across which there is a transport of particles. There are three types of shocks in MHD: slowmode, intermediate and fastmode shocks. Intermediate shocks are noncompressive (meaning that the plasma density does not change across the shock). They are also isentropic. They are sometimes referred as rotational discontinuities. All thermodynamic quantities are continuous across the shock, but the tangential component of the magnetic field can "rotate". Slowmode and fastmode shocks are compressive and are associated with an increase in entropy. Across slowmode shock, the tangential component of the magnetic field decreases. Across fastmode shock it increases. The type of shocks depend on the relative magnitude of the upstream velocity in the frame moving with the shock with respect to some characteristic speed. Those characteristic speeds, the slow and fast magnetosonic speeds, are related to the Alfvén speed, v_{A} and the sonic speed, c_{s} as follows: where V_{An} is the normal component of the Alfvénic speed. The normal component of the slow shock propagates with velocity a_{slow} in the frame moving with the upstream plasma, that of the intermediate shock with velocity V_{An} and that of the fast shock with velocity a_{fast}. Example of shocks and discontinuities in space
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This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Shocks_and_discontinuities_(magnetohydrodynamics)". A list of authors is available in Wikipedia. 