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.