Ideal diameter and length (or height) of cantenna for hydrogen line radio astronomy
For a hydrogen-line (1420.405 MHz) cantenna, the “ideal length” depends on which style of design you’re aiming for. A cantenna is really a short section of cylindrical waveguide, so its diameter matters more than its length — but length still affects efficiency and pattern.
Below is the practical answer used by radio astronomers:
⭐ 1. Waveguide Diameter (Most Important)
Cutoff frequency for circular waveguide:
fc = (1.8412 * c) / (2 * π * a)
Where:
c = 3e8 m/s
a = radius of can
fc = cutoff frequency
For the hydrogen line:
f0 = 1420.405 MHz
Best practice:
fc ≈ 0.75 to 0.80 * f0
=> fc ≈ 1.05 to 1.15 GHz
Solving gives:
diameter ≈ 150–160 mm
(About 6.0–6.25 inches).
⭐ 2. Ideal Cantenna Length
Free-space wavelength:
lambda0 = c / f0
lambda0 = 3e8 / 1.420e9
lambda0 ≈ 0.211 m (≈ 21.1 cm)
Guided wavelength λg inside the can is slightly longer:
lambda_g ≈ 24–26 cm
Rule of thumb:
ideal_length ≈ 0.5 to 1.0 * lambda_g
Therefore:
ideal_length ≈ 12–26 cm (5–10 inches)
Most hydrogen-line cans use:
18–22 cm (7–9 inches)
⭐ 3. Probe Dimensions & Position
Quarter-wave probe in free space:
lambda0 / 4 ≈ 21 cm / 4 ≈ 5.3 cm
Shortened inside waveguide:
probe_length ≈ 45–50 mm
probe_offset_from_back ≈ 45–55 mm
📌 Summary (ASCII-ready)
CAN DIAMETER: 150–160 mm (6–6.25 inches)
CAN LENGTH: 18–22 cm (7–9 inches)
LENGTH RANGE: 12–26 cm (5–10 inches)
PROBE LENGTH: 45–50 mm
PROBE OFFSET: 45–55 mm