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astronomy.me.uk The Website of Lichfield Radio Astronomy Observatory (LRO)

Astronomy observatory in Staffordshire, England.

astronomy.me.uk The Website of Lichfield Radio Astronomy Observatory (LRO)

Astronomy observatory in Staffordshire, England.

  • Live feeds at Lichfield Radio Observatory (LRO)
  • Calculators
  • Telescopes & Associated Equipment at Lichfield Radio Observatory
  • History and description of Lichfield Radio Observatory (LRO)
  • Publications & Presentations
  • Links to other observers’ SID monitoring sites
  • SHOOS – SARA Hydrogen-Observing Overall Survey
  • Contact me
Radio Interferometry

Is a shared clock required for interferometry with two software-defined radios, one per receiver?

Admin September 22, 2025 No Comments

Short answer: it depends on how you plan to combine the two channels: Practical options for your setup What to do based on your goal Why is a shared clock…

Radio observation in hydrogen line (1420MHz)

Adding second monopole onto 1420 MHz cantenna at 90 degrees to first monopole in attempt to improve signal.

Admin September 20, 2025 2 Comments

I tried adding second monopole onto 1420 MHz cantenna at 90 degrees to first monopole in attempt to improve signal, with 1.5 wavelength phasing cable on one monopole. I used…

Radio Interferometry

Open Source Tools / Libraries for interferometry

Admin September 20, 2025 No Comments

There are several open-source software tools and libraries for interferometry / correlator / radio astronomy work. Depending on how much of the pipeline you want (just correlation, calibration + imaging,…

Radio Interferometry

Concrete examples of small-scale / home interferometry projects & designing system based on SDRPlay Duo software-defined radio.

Admin September 19, 2025 No Comments

Some concrete examples of small-scale / home interferometry projects that use open-source software, so you can see how people have actually tied the pieces together. Here are some examples you…

Radio observation in hydrogen line (1420MHz)

Effect of blockage prime focus waveguide and supports on radio dish – diagrams and beam cuts

Admin September 19, 2025 No Comments

Modelling a 3 m dish at 1420.405 MHz in two ways: You’ll see: Diagrams: • Unblocked beam 2D: • Prime-focus (blocked+struts) beam 2D: • Beam cuts for 3m dish (this…

Radio observation in hydrogen line (1420MHz)

Diffraction effects on prime focus radio dishes

Admin September 19, 2025 No Comments

This comes up a lot in both radio astronomy and satellite communication when using prime-focus reflectors. On a prime-focus parabolic dish, diffraction effects mainly arise from: 1. Feed Support Legs…

Radio Interferometry

Open-source software tools and libraries for interferometry / correlator / radio astronomy

Admin September 19, 2025 No Comments

There are several open-source software tools and libraries for interferometry / correlator / radio astronomy work. Depending on how much of the pipeline you want (just correlation, calibration + imaging,…

Building radio telescopes

The “loss surface area” from a prime-focus feed

Admin September 19, 2025 No Comments

The “loss surface area” from a prime-focus feed is just the blocked (shadowed) aperture from the feed assembly (feed + support struts). You can estimate it with: So: Ablocked≈Afeed+N w D2,Fraction blocked=AblockedAdishA_\text{blocked}…

Building radio telescopes

Typical weight of plywood used to make ribs on homemade radio dish

Admin September 19, 2025 No Comments

The weight of a 6 ft × 4 ft sheet of plywood depends on its thickness and the wood species/density. Let’s go step by step: 1. Area of sheet 6…

Building radio telescopes

Typical weight of 5 ft × 5 ft sheet of fine aluminium window screening used to cover homemade radio dish

Admin September 19, 2025 No Comments

Weight of a 5 ft × 5 ft sheet of fine aluminium window screening. Let’s work it out step by step: 5 ft×5 ft=25 ft^2. 25 ft^2×0.035 lb/ft^2≈0.875 lb. That’s…

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Categories

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Recent Posts

  • What torque is required on drive to move 150cm dish?
  • Wind damage to LRO-H3
  • Online interdigital RF cavity filter designer
  • Alex Pettit’s new RFI removal regime in H-Line 3D
  • Tell me what a SID (Sudden Ionospheric Disturbance) is and what range of frequencies are covered when monitoring for SIDs.

Recent Comments

  1. Admin on Signal attenuation (loss) for common coaxial cables at around 1.42 GHz (1420 MHz), relevant for builders of amateur Hydrogen Line radio telescopes.
  2. Alex Pettit on How can a 50 ohm resistor be used to produce reference signal on a radio telescope with 50 ohm impedance?
  3. Alex Pettit on How can a 50 ohm resistor be used to produce reference signal on a radio telescope with 50 ohm impedance?
  4. Bill S.N. on How can a 50 ohm resistor be used to produce reference signal on a radio telescope with 50 ohm impedance?
  5. Stephen Arbogast on How can a 50 ohm resistor be used to produce reference signal on a radio telescope with 50 ohm impedance?

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You missed

Uncategorized

What torque is required on drive to move 150cm dish?

Uncategorized

Wind damage to LRO-H3

Uncategorized

Online interdigital RF cavity filter designer

Uncategorized

Alex Pettit’s new RFI removal regime in H-Line 3D

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astronomy.me.uk The Website of Lichfield Radio Astronomy Observatory (LRO)

Astronomy observatory in Staffordshire, England.

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