Polarization by Reflection — Question 9

Section 33-9 · Physics pages 5548–5549

Question 9 Small angular error produces quadratic p leakage near Brewster incidence For air-to-index-n incidence, use rp = (n cos i −cos t)/(n cos i + cos t) and sin i = n sin t, with n greater than one. Set i = θB + δ, where θB = tan−1 n and delta is small in radians. δ Rp Brewster Schematic; labels, not drawing lengths, specify the data. (a) Differentiate at Brewster incidence to find the leading reflected amplitude. (b) Find the leading power reflectance and estimate it for n=1.50 and delta=1.0 degree.
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Question 9 - Solution Small angular error produces quadratic p leakage near Brewster incidence δ Rp Brewster (a) Method and calculation dt di B = cos θB n cos tB = 1 n2 . drp di B = −n sin θB + sin tB/n2 2n cos θB = −n4 −1 2n3 . (b) Interpretation and further calculation rp ≃−n4 −1 2n3 δ, Rp ≃ n4 −1 2n3 !2 δ2 . δ = π/180 : Rp ≃1.10340 × 10−4 ; Rp(2δ) ≃4Rp(δ). Physical check The amplitude crosses zero linearly while its squared magnitude has a quadratic minimum. The estimate neglects higher orders in angular error.

Question 9

Small angular error produces quadratic p leakage near Brewster incidence

For air-to-index-n incidence, use rp=(ncos⁡i−cos⁡t)/(ncos⁡i+cos⁡t)r_p=(n\cos i-\cos t)/(n\cos i+\cos t) and sin⁡i=nsin⁡t\sin i=n\sin t, with n greater than one. Set i=θB+δi=\theta_B+\delta, where θB=tan⁡−1n\theta_B=\tan^{-1}n and delta is small in radians.

Diagram shown in the original SVG worksheet.

  1. Differentiate at Brewster incidence to find the leading reflected amplitude.

  2. Find the leading power reflectance and estimate it for n=1.50 and delta=1.0 degree.

Question 9 - Solution

Small angular error produces quadratic p leakage near Brewster incidence

Diagram shown in the original SVG worksheet.

(a) Method and calculation

dtdi|B=cos⁡θBncos⁡tB=1n2.\left.\frac{dt}{di}\right|_B=\frac{\cos\theta_B}{n\cos t_B}=\frac1{n^2}.drpdi|B=−nsin⁡θB+sin⁡tB/n22ncos⁡θB=−n4−12n3.\left.\frac{dr_p}{di}\right|_B=\frac{-n\sin\theta_B+\sin t_B/n^2}{2n\cos\theta_B}=\boxed{-\frac{n^4-1}{2n^3}}.

(b) Interpretation and further calculation

rp≃−n4−12n3δ,Rp≃(n4−12n3)2δ2.\boxed{r_p\simeq-\frac{n^4-1}{2n^3}\delta,\quad R_p\simeq\left(\frac{n^4-1}{2n^3}\right)^2\delta^2}.δ=π/180:Rp≃1.10340×10−4;Rp(2δ)≃4Rp(δ).\delta=\pi/180:\quad\boxed{R_p\simeq1.10340\times10^{-4}};\quad R_p(2\delta)\simeq4R_p(\delta).

Physical check

The amplitude crosses zero linearly while its squared magnitude has a quadratic minimum. The estimate neglects higher orders in angular error.