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Distribution functions in velocity in a collisiondominated mirror plasma can be obtained numerically by solving the appropriate Fokker-Planck equations 1. Under well-tested assumptions 2,3 these equations a r e azimuthally invariant and approximately separable in the v and 6 components of velocity, where , u ≡ cos θ = v∥ /v and v∥ is in the direction of the local mirror field.
John P. Holdren (Wed,) studied this question.