The origin of the dynamo velocity field of the reversed field pinch within the visco-resistive MHD modeling is uncovered. The main component of this field is an electrostatic drift. The corresponding electrostatic field is related to a small charge separation which is consistent with the quasineutrality approximation, and which should be present in real plasmas, too. While quite natural in the stationary single helicity state, this analysis is shown to extend also to the nonstationary multiple helicity regime. Numerical simulations provide the spatial distribution of fields and of charge separation.

Dominant Electrostatic Nature of the Reversed Field Pinch Dynamo

Bonfiglio D;S Cappello;
2005

Abstract

The origin of the dynamo velocity field of the reversed field pinch within the visco-resistive MHD modeling is uncovered. The main component of this field is an electrostatic drift. The corresponding electrostatic field is related to a small charge separation which is consistent with the quasineutrality approximation, and which should be present in real plasmas, too. While quite natural in the stationary single helicity state, this analysis is shown to extend also to the nonstationary multiple helicity regime. Numerical simulations provide the spatial distribution of fields and of charge separation.
2005
Istituto gas ionizzati - IGI - Sede Padova
Inglese
94
145001
4
http://prl.aps.org/abstract/PRL/v94/i14/e145001
Sì, ma tipo non specificato
MHD modeling
dynamo effect
nonlinear phenomena
self-organization
2
info:eu-repo/semantics/article
262
Bonfiglio D.; S. Cappello; D. F. Escande
01 Contributo su Rivista::01.01 Articolo in rivista
none
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/53067
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