Radio observation in hydrogen line (1420MHz)

Optimising the feed for 2m dish used for hydrogen line radio astronomy

ChatGPT suggested following April 2025:

Great — optimizing the feed for your 2 m dish at 1420 MHz will ensure you’re getting the most out of your improved collecting area and resolution. Here’s what we need to cover:


1. Focal Length Calculation

For a typical parabolic dish:

  • Focal length (f) is often about 0.25 to 0.45 × D depending on the dish shape (deep vs shallow).
  • If your dish is prime focus and shaped similarly to your 1.5 m dish, a safe estimate is:
    • f/D ≈ 0.35 → f ≈ 0.35 × 2.0 m = 0.70 m

You can confirm focal length by physical measurement or by sunlight burn focus at noon.


2. Feed Type

At 1420 MHz (λ ≈ 21.1 cm), good feed options include:

  • Half-wave dipole + reflector at focus
  • Sleeve dipole (to broaden beam pattern)
  • Small pyramidal horn
  • Cantenna (waveguide open-ended cylinder)
  • Scalar feedhorn (best, but complex)

If your previous 1.5 m dish used a dipole and reflector, you can scale it or adjust spacing slightly for the new focal length.


3. Dipole + Reflector Feed Example

This simple setup can work well for a 2 m dish:

  • Dipole length:
    0.49 λ = 10.3 cm (free space, adjust shorter if near metal or for matching)
  • Reflector:
    Flat metal plate (20–25 cm square or round), placed about 0.25 λ (~5.3 cm) behind the dipole
  • Orientation:
    Mount at the focal point, perpendicular to the incoming rays
  • Balun/matching:
    Use a coax balun (e.g., 1:1 choke or quarter-wave transformer) for impedance match to 50 Ω cable

4. Illumination and Spillover

  • Your feed should illuminate the dish evenly, with about -10 dB drop at the edge.
  • If the beam is too narrow, you’ll under-illuminate (low gain); too wide, and you’ll get spillover and ground noise.

Dipole + reflector setups naturally give ~60° beamwidth, which suits f/D ≈ 0.35–0.4 dishes well.


5. Next Steps

If you like, I can:

  • Provide a sketch/schematic of a dipole + reflector feed
  • Simulate or model the beam pattern for your f/D
  • Help you design a waveguide or horn feed (e.g., WR-650 section or custom)

Absolutely — let’s do both. Here’s a breakdown of the dipole + reflector feed and a WR-650 waveguide feed suitable for your 2 m dish at 1420 MHz. I’ll follow with diagrams for each.


1. Dipole + Reflector Feed (Simple, Effective)

Key Dimensions:

  • Frequency: 1420 MHz → λ ≈ 21.1 cm
  • Dipole length (L): ~0.49 λ → 10.3 cm total (5.15 cm each arm)
  • Reflector spacing (S): ~0.25 λ → 5.3 cm
  • Reflector size: ≥ λ × λ → 25 × 25 cm metal plate
  • Mounting: Centered at focal point (about 70 cm from dish vertex), dipole horizontal.

Notes:

  • Use RG-58 or RG-6 coax with a 1:1 choke balun (e.g., 4–5 turns of coax through ferrite)
  • Match carefully to avoid VSWR degradation

2. WR-650 Waveguide Feed (Better pattern, More Directional)

WR-650 Specs:

  • Standard waveguide for 1.12–1.7 GHz
  • Internal dimensions: 165.1 mm × 82.55 mm
  • Cutoff for TE10 ≈ 892 MHz (well within band)
  • Good impedance match for 1420 MHz

Feed Design:

  • Use a ~15–20 cm section as a waveguide horn
  • Place thin λ/4 probe (~5 cm) into the broad wall for coax connection
  • For beam shaping: add a conical or rectangular flare (or scalar ring)

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