Energy Transport and the Poynting Vector — Question 1

Section 33-4 · Physics pages 5432–5433

Question 1 Peak field and rms field give the same time-averaged energy flux A sinusoidal vacuum plane wave has electric amplitude E0 = 150 V/m. Use ϵ0 = 8.854 × 10−12 F/m and c = 3.00 × 108 m/s. A flat detector of area A = 2.0 × 10−3 square meters has its normal 60 degrees from propagation. S ˆn Schematic; labels, not drawing lengths, specify the data. (a) Find rms electric field, intensity, and mean total energy density. (b) Find the average power crossing the detector and explain which area enters the flux.
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Question 1 - Solution Peak field and rms field give the same time-averaged energy flux S ˆn (a) Method and calculation Erms = E0/ √ 2 = 106.066 V/m, I = ϵ0cE2 rms = 29.8823 W/m2 . ⟨u⟩= I/c = 9.96075 × 10−8 J/m3 . (b) Interpretation and further calculation P = ⟨S⟩· ˆnA = IA cos 60◦. P = 2.98823 × 10−2 W ; A⊥= A cos 60◦. Physical check The intensity is defined per area perpendicular to propagation, while the physical detector area is tilted.

Question 1

Peak field and rms field give the same time-averaged energy flux

A sinusoidal vacuum plane wave has electric amplitude E0=150E_0=150 V/m. Use ϵ0=8.854×10−12\epsilon_0=8.854\times10^{-12} F/m and c=3.00×108c=3.00\times10^8 m/s. A flat detector of area A=2.0×10−3A=2.0\times10^{-3} square meters has its normal 60 degrees from propagation.

Diagram shown in the original SVG worksheet.

  1. Find rms electric field, intensity, and mean total energy density.

  2. Find the average power crossing the detector and explain which area enters the flux.

Question 1 - Solution

Peak field and rms field give the same time-averaged energy flux

Diagram shown in the original SVG worksheet.

(a) Method and calculation

Erms=E0/2=106.066V/m,I=ϵ0cErms2=29.8823W/m2.E_{\mathrm{rms}}=E_0/\sqrt2=106.066\,\mathrm{V/m},\quad I=\epsilon_0cE_{\mathrm{rms}}^2=\boxed{29.8823\,\mathrm{W/m^2}}.⟨u⟩=I/c=9.96075×10−8J/m3.\boxed{\langle u\rangle=I/c=9.96075\times10^{-8}\,\mathrm{J/m^3}}.

(b) Interpretation and further calculation

P=⟨𝑺⟩⋅n̂A=IAcos⁡60∘.P=\langle\mathbf S\rangle\cdot\hat n A=IA\cos60^\circ.P=2.98823×10−2W;A⟂=Acos⁡60∘.\boxed{P=2.98823\times10^{-2}\,\mathrm W};\quad A_\perp=A\cos60^\circ.

Physical check

The intensity is defined per area perpendicular to propagation, while the physical detector area is tilted.