The equation (??) for kρ has two solutions corresponding to inward and outward propagating waves. The solution is chosen such that the ray initially propagates inward, meaning
| (64) |
We have
| (65) |
where
| (66) |
since N∥ is independent of kρ. For positive energy waves with ∂∕∂ω > 0 the condition (??) thus becomes,
| (67) |
We have (??)
| (68) |
In general > such that (??) reduces to
| (69) |
or equivalently
| (70) |
where S⊥ is the energy flow density in the perpendicular direction.