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Limits on plasma anisotropy in a tail‐like magnetic field
Author(s) -
Hill T. W.,
Voigt G.H.
Publication year - 1992
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/92gl02497
Subject(s) - anisotropy , physics , isotropy , plasma , magnetic field , field (mathematics) , symmetry (geometry) , field strength , tensor (intrinsic definition) , plasma sheet , plane (geometry) , computational physics , geometry , magnetosphere , optics , quantum mechanics , mathematics , pure mathematics
The condition of magnetohydrostatic equilibrium implies tight constraints on the degree of anisotropy that is supportable in a magnetotail field geometry. If the plasma pressure tensor is assumed to be gyrotropic at the tail midplane ( z =0), then equilibrium requires that it also be nearly isotropic there, with P ⟂o / P //o in the range 1 ± δ 2 where δ∼0.1 is the ratio of the normal field component at the symmetry plane to the field strength in the tail lobe. The upper and lower limits are essentially equivalent, respectively, to the marginal mirror and firehose stability conditions evaluated at z=0, which have been invoked previously to limit the degree of anisotropy in the plasma sheet.