PHYSICS · Multi-part · Fermi University Physics · Electricity, Magnetism & Electromagnetism · Plasma Physics · Waves in plasmas
Modes, Packets and Media, Ch Transmission lines and electromagnetic waves in matter, plasmas and guides
Problem
A radio-astronomy receiver observes a pulsar. Its dipole feed presents a resistive impedance ZL=300Ω and is matched to the Z0=50Ω coaxial line of the receiver by a quarter-wave transformer designed for f0=800MHz, built from a coaxial line with velocity factor 0.70, giving a wave speed of 0.70c in the transformer.
((a)) Find the transformer's characteristic impedance Zm and its physical length ℓ.
((b)) The receiver specification requires the voltage reflection coefficient at the 50Ω input, Γ=(Zin−Z0)/(Zin+Z0), to satisfy ∣Γ∣≤0.10 down to 750MHz. Using the general (not the quarter-wave-only) input-impedance formula for a lossless line of length ℓ and characteristic impedance Zm terminated in ZL, find ∣Γ∣ at 750MHz and state whether the specification is met.
((c)) The pulsar's radiation crosses about 1.5kpc of interstellar plasma whose mean electron density gives a plasma frequency of order 1.3kHz, far below the 400-800MHz band used here. Using the free electron's equation of motion, explain (i) why this plasma does not measurably absorb the signal at these frequencies, and (ii) why, if a wave's frequency were instead below the plasma frequency, the same plasma would turn it back completely rather than absorb it.
((d)) A two-channel spectrogram of one pulse shows the 800MHz channel leading the 400MHz channel by 584ms. Taking the source distance as D=1.5kpc, find the dispersion measure and the mean electron density along the path, and state briefly why the delay scales as 1/f2 rather than 1/f.