Magnetic holes in plasmas close to the mirror instability
Non-propagating magnetic hole solutions in anisotropic plasmas near the mirror instability threshold are investigated in numerical simulations of a fluid model that incorporates linear Landau damping and finite Larmor radius corrections calculated in the gyrokinetic approximation. This FLR-Landau fl...
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Published in | Nonlinear processes in geophysics Vol. 14; no. 4; pp. 373 - 383 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
Gottingen
Copernicus GmbH
01.01.2007
European Geosciences Union (EGU) Copernicus Publications |
Subjects | |
Online Access | Get full text |
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Summary: | Non-propagating magnetic hole solutions in anisotropic plasmas near the mirror instability threshold are investigated in numerical simulations of a fluid model that incorporates linear Landau damping and finite Larmor radius corrections calculated in the gyrokinetic approximation. This FLR-Landau fluid model reproduces the subcritical mirror bifurcation recently identified on the Vlasov-Maxwell system, both by theory and numerics. Stable magnetic hole solutions that display a polarization different from that of Hall-MHD solitons are indeed obtained slighlty below threshold, while magnetic patterns and spatio-temporal chaos emerge when the system is maintained in a mirror unstable regime. |
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Bibliography: | ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 1607-7946 1023-5809 1607-7946 |
DOI: | 10.5194/npg-14-373-2007 |