Radiative transfer dynamo effect

Munirov, Vadim R.; Fisch, Nathaniel J.

doi:10.1103/PhysRevE.95.013205

Title: Radiative transfer dynamo effect

Journal Article · 17 January 2017 · Physical Review E

DOI: https://doi.org/10.1103/PhysRevE.95.013205 · OSTI ID:1344115

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Princeton Univ., Princeton, NJ (United States). Princeton Plasma Physics Lab. and Dept. of Astrophysical Sciences

Here, 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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Research Organization:: Princeton Plasma Physics Laboratory (PPPL), Princeton, NJ (United States)

Sponsoring Organization:: USDOE Office of Science (SC), Fusion Energy Sciences (FES); USDOE

Grant/Contract Number:: AC02-09CH11466; AC02-09CH1-1466

OSTI ID:: 1344115

Alternate ID(s):: OSTI ID: 1339781

Journal Information:: Physical Review E, Vol. 95, Issue 1; ISSN 2470-0045

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 5 works

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Cited By (2)

Radiation in equilibrium with plasma and plasma effects on cosmic microwave background Munirov, Vadim R.; Fisch, Nathaniel J. Physical Review E, Vol. 100, Issue 2 https://doi.org/10.1103/physreve.100.023202	journal	August 2019
Radiation in equilibrium with plasma and plasma effects on cosmic microwave background Munirov, Vadim R.; Fisch, Nathaniel J. arXiv https://doi.org/10.48550/arxiv.1903.05616	text	January 2019

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Title: Radiative transfer dynamo effect

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