The multifluid character of the ``Baranov'' interface (Q5931489)

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scientific article; zbMATH DE number 1591179
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The multifluid character of the ``Baranov'' interface
scientific article; zbMATH DE number 1591179

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    The multifluid character of the ``Baranov'' interface (English)
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    2 July 2001
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    The interaction of the solar system with an ambient interstellar medium flow is characterized by its hydrodynamic nature invoking structures like inner shock, heliopause and outer shock with plasma sheath regions in between. The author shows how the main features of this interaction change if its multifluid character is taken into account.
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    space plasma
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    Baranov interface
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    multifluid flow
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    solar system
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    ambient interstellar medium flow
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    inner shock
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    heliopause
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    outer shock
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    plasma sheath
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