``Thermal layer'' effect in MHD: Interaction of a parallel shock with a layer of decreased density (Q1312613)
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scientific article; zbMATH DE number 493621
| Language | Label | Description | Also known as |
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| English | ``Thermal layer'' effect in MHD: Interaction of a parallel shock with a layer of decreased density |
scientific article; zbMATH DE number 493621 |
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``Thermal layer'' effect in MHD: Interaction of a parallel shock with a layer of decreased density (English)
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27 April 1994
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Interaction of a parallel fast MHD shock with a layer of decreased density is discussed using ideal MHD approach. This is an extrapolation of gas dynamic ``thermal layer'' effect on ideal MHD. This problem appears in connection with cosmical shock propagation where planetary magnetic tails play the role of the ``thermal layer'', and it may also be observed in the laboratory when the shock is strong enough to heat the walls ahead of it.
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computer simulation
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cosmical shock propagation
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planetary magnetic tails
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