1971
DOI: 10.1088/0032-1028/13/9/009
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Transport equations and gradient instabilities in a high pressure collisional plasma

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Cited by 96 publications
(116 citation statements)
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“…(24). Like the ∇⋅ r q || − 3 r n⋅∇ r q || ⋅ r n term, they have small coefficients, but are formally of the same order as the remaining terms previously obtained by Mikhailovskii and Tyspin [4][5][6]. Indeed, the r q || ⋅∇T and q || 2 are exactly of the same form and so can be combined to write t π || = ( r n r n − 1 3…”
Section: Ion Viscosity and Collisional Perpendicular Ion Heat Fluxmentioning
confidence: 73%
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“…(24). Like the ∇⋅ r q || − 3 r n⋅∇ r q || ⋅ r n term, they have small coefficients, but are formally of the same order as the remaining terms previously obtained by Mikhailovskii and Tyspin [4][5][6]. Indeed, the r q || ⋅∇T and q || 2 are exactly of the same form and so can be combined to write t π || = ( r n r n − 1 3…”
Section: Ion Viscosity and Collisional Perpendicular Ion Heat Fluxmentioning
confidence: 73%
“…The solution for f 2 contains terms of order δ 2 and δ ∆ ; the order ν/Ω perpendicular viscosity corrections will be evaluated by a moment approach in the next section. Our solution differs from that of Mikhailovskii and Tsypin [4][5][6] who use a polynomial approximation for f 2 that neglects terms involving L 2…”
Section: Ion Formulationmentioning
confidence: 93%
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