Fluctuation dynamo in a collisionless, weakly magnetized plasma
Results from a numerical study of fluctuation dynamo in a collisionless, weakly magnetized plasma are presented. The key difference between this dynamo and its magnetohydrodynamic (MHD) counterpart is the adiabatic production of magnetic-field-aligned pressure anisotropy by the amplification of a we...
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| Format: | Journal article |
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American Astronomical Society
2018
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