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Transmission and damping of hydromagnetic waves behind a strong shock front: implications for cosmic ray acceleration - MaRDI portal

Transmission and damping of hydromagnetic waves behind a strong shock front: implications for cosmic ray acceleration (Q3779939)

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Transmission and damping of hydromagnetic waves behind a strong shock front: implications for cosmic ray acceleration
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    Transmission and damping of hydromagnetic waves behind a strong shock front: implications for cosmic ray acceleration (English)
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    1986
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    Acceleration of cosmic rays
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    Fermi mechanism
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    intergalactic shock waves
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    low-frequency Alfvén waves
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    transmission
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    high beta plasma
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    Long wave length modes
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    scattering highly relativistic ions
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    particle acceleration
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    wave turbulence
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    firehose instabilities
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    post-shock turbulence
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