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Universal interchange instability in partially ionized gases

Journal Article · · Physics of Fluids B; (USA)
DOI:https://doi.org/10.1063/1.859378· OSTI ID:6314305
 [1]
  1. Space Plasma Branch, Plasma Physics Division, Naval Research Laboratory, Washington, DC 20375-5000 (USA)

A magnetized, inhomogeneous, partially ionized gas is theoretically shown to be unstable to an interchange instability. The source of free energy for the instability is the cross-field current. The instability is caused by neutral drag dynamics, and is therefore critically dependent upon charged particle--neutral collisions {nu}{sub {alpha}{ital n}}. The growth rate is largest in the strongly coupled regime, i.e., {omega}{much lt}{nu}{sub {ital in}}, {nu}{sub {ital ni}}, and is given by {gamma}{congruent}({epsilon}{ital m}{sub {ital e}}/{ital m}{sub {ital i}}){sup 1/2}(1+{epsilon}){sup {minus}1}{ital k}{sub {ital y}}{ital V}{sub {ital d}}, where {ital k}{sub {ital y}} is the wave number, {ital V}{sub {ital d}}=({ital cT}/{ital eB})({partial derivative} ln({ital n}{sub {ital i}0})/{partial derivative}{ital x}) is the diamagnetic drift velocity, {ital T}={ital T}{sub {ital e}}+{ital T}{sub {ital i}}, and {epsilon}={ital m}{sub {ital n}}{ital n}{sub {ital n}}/{ital m}{sub {ital i}}{ital n}{sub {ital i}} ({ital m} is the mass and {ital n} the density of the ions ({ital i}) and neutrals ({ital n})). The growth rate is a maximum when {epsilon}=1, which corresponds to {nu}{sub {ital in}}={nu}{sub {ital ni}}.

OSTI ID:
6314305
Journal Information:
Physics of Fluids B; (USA), Journal Name: Physics of Fluids B; (USA) Vol. 2:11; ISSN 0899-8221; ISSN PFBPE
Country of Publication:
United States
Language:
English