Radiative transfer dynamo effect. 2017

Vadim R Munirov, and Nathaniel J Fisch
Princeton Plasma Physics Laboratory, Princeton University, Princeton, New Jersey 08543, USA and Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08540, USA.

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.

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