For a real scalar wave equation , the next order of the WKB approximation gives . Thus , and the leading Wronskian flux of a right-travelling component is independently of the local wavenumber.
Let . The WKB approximation in the barrier can be rewritten as
The right Airy turning-point connection formula gives
so and . Impose no incident wave from the right, . Then
Consequently, within the leading Airy turning-point connection formula calculation,
For an opaque barrier, ,
The transmission coefficient is a ratio of Poynting fluxes; the normalization already includes their local wavenumber factors. The displayed denominator is useful for consistent matching and Wronskian flux conservation, but does not claim accuracy for subleading terms beyond the WKB approximation, or for merging wave turning points.
For real , the wave equation has the conserved Wronskian flux
For this ordinary plasma wave, the time-averaged Poynting flux is . With no incident wave from the right, evaluating the same Wronskian flux on both sides proves
The coefficients in f also satisfy this identity algebraically, before the opaque-barrier expansion.
A plasma wave resonance makes the ideal cold description singular and requires an appropriate causal regularization. A passive resonant layer can absorb wave energy into particle motion, or convert it into another branch. For the two measured outgoing channels one then has
with when resonant absorption or uncounted mode conversion occurs. A numerical value of requires the layer physics; a resonance by itself does not specify a universal loss fraction. Counting all converted and absorbed energy preserves conservation of energy.