Question 4 of 8: Polarization of Two Orthogonal Plane Waves
Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)
Notes on this paper
98-Phys-A3, Electromagnetics — National Exam, December 2016. 3-hour closed-book exam (Casio or Sharp approved calculators only); any FIVE of the eight questions constitute a complete paper and only the first five as they appear in a candidate's answer book are marked, each of equal value. Aids given on the paper: ε0 = 8.85×10-12 F/m, μ0 = 4π×10-7 H/m. All eight printed questions are solved below as a complete study resource.
Reference texts: Sadiku, Elements of Electromagnetics (7th ed.) — transmission lines, waveguides, plane waves, antennas; Hayt & Buck, Engineering Electromagnetics (9th ed.) — transmission-line transients; Pozar, Microwave Engineering (4th ed.) — transmission-line theory and stub matching; Balanis, Antenna Theory (4th ed.) — short-dipole far field.
Question 4: Polarization of Two Orthogonal Plane Waves (equal value)
Given. Two 10 GHz plane waves in free space, equal power density $S=1\ \text{W/m}^2$ each; wave 1 travels due north with $\mathbf E_1$ horizontal (east–west); wave 2 travels due east with $\mathbf E_2$ vertical; at point A the two fields are in phase (given: total field linear).
Find. (i) RMS amplitude of the total field at A; (ii) the nearest point to A where the total field is circularly polarized.
Wave 1's $\mathbf E$ (east–west) and wave 2's $\mathbf E$ (vertical) are mutually perpendicular at A; moving diagonally (NW/SE) shifts their relative phase fastest.
Approach. Get each wave's RMS field from $S=E_{rms}^2/\eta_0$; because $\mathbf E_1\perp\mathbf E_2$ and they are in phase at A, the resultant magnitude is the vector sum of two equal, orthogonal, in-phase components. For part (ii), each wave's phase depends only on distance travelled along its OWN propagation direction, so move away from A in the direction that changes the two waves' relative phase fastest — the diagonal (NW/SE) direction — until that phase difference reaches $90^\circ$.
RMS field of one wave. $$E_0=\sqrt{S\,\eta_0}=\sqrt{(1)(376.8)}=19.41\ \text{V/m}.$$
Total field at A. $\mathbf E_1$ and $\mathbf E_2$ are equal in magnitude, mutually perpendicular (east–west vs. vertical), and in phase at A, so they add as perpendicular vectors:
$$E_{rms}=\sqrt{E_1^2+E_2^2}=E_0\sqrt2=\boxed{27.45\ \text{V/m}}.$$
Phase gradient toward circular polarization. With north $=\hat x$, east $=\hat y$, wave 1's phase is $kx$ and wave 2's is $ky$ ($k=2\pi/\lambda$), so their relative phase is $\Delta\phi=k(x-y)$. This changes fastest per unit distance moved along the diagonal $(\hat x-\hat y)/\sqrt2$ (NW), at rate $k\sqrt2$ per metre. Circular polarization needs $|\Delta\phi|=90^\circ=\pi/2$ relative to A (which starts at $\Delta\phi=0$, linear):
$$d=\frac{\pi/2}{k\sqrt2}=\frac{\lambda}{4\sqrt2}.$$
Evaluate. $\lambda=c/f=(3\times10^8)/(10\times10^9)=0.03$ m, so
$$d=\frac{0.03}{4\sqrt2}=\boxed{5.30\ \text{mm}}.$$
This distance applies in EITHER diagonal sense: $5.30$ mm to the north-west of A gives $\Delta\phi=+90^\circ$ (one circular sense), and $5.30$ mm to the south-east gives $\Delta\phi=-90^\circ$ (the opposite sense) — both are equally the "nearest" point.
Field at A and nearest circular-polarization point