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introduction to gyrokinetic and fluid simulations of ... - Our Home Page

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The Nonlinear Gyrokinetic Equation<br />

Guiding center distribution function Fs(x, v, t) = F0s(ψ, W ) + F0s(ψ, W )qs ˜ φ/Ts +<br />

˜hs(x, W, µ, t) = equilibrium + fluctuating components, where the energy W =<br />

mv 2 + µB, the first adiabatic invariant µ = mv 2 ⊥/B, <strong>and</strong><br />

∂ ˜ hs<br />

∂t<br />

∂ ˜χ<br />

∂W ∂t<br />

+ Collisions + Sources + Sink<br />

<br />

<br />

+ ˜vχ + v ˆ<br />

b + vd · ∇˜ hs = −˜ ∂F0s<br />

vχ · ∇F0s − qs<br />

where ˆ b points in the direction <strong>of</strong> the equilibrium magnetic field, v d is the curvature<br />

<strong>and</strong> grad B drift, Ωs is the gyr<strong>of</strong>requency, <strong>and</strong> the ExB drift is combined with<br />

transport along perturbed magnetic fields lines <strong>and</strong> the perturbed ∇B drift as:<br />

˜vχ = c<br />

B ˆ <br />

b × ∇ ˜χ ˜χ = J0(γ) ˜φ − v c à <br />

<br />

+ J1(γ) mv<br />

γ<br />

2 ⊥<br />

e<br />

J0 & J1 are Bessel functions with γ = k ⊥v⊥/Ωs, <strong>and</strong> the fields are from<br />

0 ≈ 4π <br />

s qs<br />

<br />

d 3 v<br />

∇ 2 Ã = − 4π <br />

c<br />

˜B 4π<br />

= −<br />

B B2 <br />

<br />

s<br />

⎡<br />

⎣qs ˜ φ ∂F0s<br />

s qs<br />

<br />

∂W + J0(γ) ˜ hs<br />

d 3 vv J0(γ) ˜ hs<br />

d 3 vmv 2 ⊥<br />

J1(γ)<br />

γ ˜ hs<br />

⎤<br />

⎦<br />

˜B <br />

B

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