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Radiative transfer dynamo effect
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DOI：10.1103/PhysRevE.95.013205.png)
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Abstract
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Magnetic fields in rotating and radiating astrophysical plasma can be produced due to a radiative interaction between plasma layers moving relative to each other. The efficiency of current drive, and with it the associated dynamo effect, is considered in a number of limits. It is shown here, however, that predictions for these generated magnetic fields can be significantly higher when kinetic effects, previously neglected, are taken into account.
Keywords:
MAGNETIC-FIELDS
COSMIC BATTERY
CURRENT GENERATION
CURRENT DRIVE
ACCRETION
PLASMA
ORIGIN
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