2004
DOI: 10.1016/j.cpc.2004.06.059
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Hybrid kinetic-MHD simulations in general geometry

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Cited by 25 publications
(48 citation statements)
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“…in the current-coupling scheme (28)- (31), so that Lorentz forces in (28) are replaced by a relative pressure term. Notice that the static equilibria of the above equations (62)-(64) coincide with those of the hybrid model in [23,43] (for hot particles undergoing Vlasov dynamics), provided the equilibrium Vlasov distribution (usually denoted by f 0 ) is isotropic in the velocity coordinate, i.e. K 0 = v f 0 d 3 v = 0.…”
Section: Formulation Of the Modelmentioning
confidence: 91%
“…in the current-coupling scheme (28)- (31), so that Lorentz forces in (28) are replaced by a relative pressure term. Notice that the static equilibria of the above equations (62)-(64) coincide with those of the hybrid model in [23,43] (for hot particles undergoing Vlasov dynamics), provided the equilibrium Vlasov distribution (usually denoted by f 0 ) is isotropic in the velocity coordinate, i.e. K 0 = v f 0 d 3 v = 0.…”
Section: Formulation Of the Modelmentioning
confidence: 91%
“…As follows from Eq. (19), the inequality (21) implies that one of the conditions for stability is that the equilibrium flow be sub-Alfvénic. Condition (22) is a sufficient condition for stability, but a more in-depth analysis would show that the line bending term can add a positive contribution.…”
Section: Energy-casimir Stability Via the Second Variationmentioning
confidence: 99%
“…, which emphasizes the various kinetic energy contributions. A natural consequence of this kinetic equation is that its zero-th moment n satisfies the simple advection relation ∂ t n + div(n U ) = 0, so that the total density D = ρ + n satisfies the equation ∂ t D + div(D U ) = 0, as it appears in [21].…”
Section: Second Pressure-coupling Schemementioning
confidence: 99%