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using
B = ∇Ψ ×∇ϕ + g∇ϕ |
![]() | (103) |
Noting that both ∇B and κ are approximatedly along − direction, which is perpendicular to ∇ϕ, Eq.
(103) is written as
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if
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then the drift from the local magnetic surface is outward, otherwise, the drift is inward.
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Examining the right-hand side of Eq. (5.8), we find that Bp and (Ψlcfs − Ψaxis) change signs simutaneouslly when the toroidal plasma current Iϕ change sign, thus the direction of Bp(Ψlcfs − Ψaxis) is independent of the sign of Iϕ. Therefore the sign of the radial drift is independent of the sign of Iϕ.