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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 Astronomy

How an inductor works

Admin November 27, 2025 No Comments

An inductor is one of the simplest components in electronics, but its behaviour comes from a deep physical effect: a current creates a magnetic field, and changing that current induces…

Radio Astronomy

How resonant radio frequency circuits work

Admin November 27, 2025 No Comments

How Resonant RF Circuits Work: Resonant RF (radio-frequency) circuits—also called LC resonant or tuned circuits—use an inductor (L) and a capacitor (C) to create a natural oscillation at a specific…

Radio observation in hydrogen line (1420MHz)

How does the radio frequency SAW filter in a Nooelec SAWBird LNA and filter?

Admin November 26, 2025 No Comments

In the SAWBird line of LNAs (e.g., for 1420 MHz, GPS, L-band), the SAW filter is the component that provides the ultra-narrow preselection that makes these modules so effective for…

Radio observation in hydrogen line (1420MHz)

What is spillover vs ground reflection in radio astronomy?

Admin November 26, 2025 No Comments

In a radio telescope’s noise budget, spillover and ground reflection are two distinct ways unwanted radiation enters your receiver. They’re related but not the same: Spillover Spillover is receiver noise…

Linux for Radio Astronomy

How to generate a disc image from my Raspberry PI 4B?

Admin November 26, 2025 No Comments

You can get a Raspberry Pi disk image in a few different ways depending on what you mean: 1. Downloading an official Raspberry Pi OS image If you simply want…

Aerials & Antennae

What difference does choice of material make with regards to construction of antennas?

Admin November 24, 2025 No Comments

Material choice affects an antenna’s efficiency, bandwidth, durability, and mechanical practicality. Here’s a concise breakdown of what really matters: 1. Electrical Conductivity This is the biggest factor. High-conductivity metals (copper,…

Radio observation in hydrogen line (1420MHz)

Is it benefitial to ensure that low noise amplifier and filter (LNA) for hydrogen line observing is at a constant temperature?

Admin November 24, 2025 No Comments

Andrew Thornett: I could see potential benefit for having LNA at constant temperature. The easiest way to achieve that is to cool it below any likely outside temperature – avoiding…

Radio observation in hydrogen line (1420MHz)

What is most expensive low noise amplifier and/or filter available for hydrogen line radio astronomy?

Admin November 24, 2025 No Comments

Short answer: the most expensive single-component front-end parts used for 1.420 GHz (H-line) work are cryogenic HEMT/InP LNAs and the associated cryogenic front-end systems (LNA + cryostat + cryocooler). Top…

Pulsars

Pulsars don’t have a single “pulsar frequency” the way spectral lines do.

Admin November 24, 2025 No Comments

Pulsars don’t have a single “pulsar frequency” the way spectral lines do — instead they emit broadband radio noise with periodic pulses, and what we observe are: Here are the…

USRP B210 Software-Defined Radio

Device addresses (USRP B210 Software-defined radio) on LRO-24 on 22/11/2025

Admin November 23, 2025 No Comments

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Categories

  • ADVISORY NOTICE & DISCLAIMER
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  • My interests in astronomy
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  • Nooelec SAWBird LNAs
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  • Radio observation in hydrogen line (1420MHz)
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  • The 20 Metre Skynet Radio Dish at Green Bank Observatory
  • Uncategorized
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Recent Posts

  • When making a VLF loop antenna to monitor SIDs, do you get better signal using less copper wire but on a bigger frame?
  • Very Low Frequency (VLF) Aerials at Lichfield Radio Observatory (LRO)
  • Latest Spectrum Lab USR settings file that works successfully with LRO 134cm VLF aerial with direct input into USB soundcard and Spectrum Lab Software as of 16/3/2026
  • How long does a photon take to cross 10cm space?
  • What amateur deep space network groups are picking up signals from deep space probes?

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

When making a VLF loop antenna to monitor SIDs, do you get better signal using less copper wire but on a bigger frame?

Uncategorized

Very Low Frequency (VLF) Aerials at Lichfield Radio Observatory (LRO)

Uncategorized

Latest Spectrum Lab USR settings file that works successfully with LRO 134cm VLF aerial with direct input into USB soundcard and Spectrum Lab Software as of 16/3/2026

Uncategorized

How long does a photon take to cross 10cm space?

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

Astronomy observatory in Staffordshire, England.

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