Skip to content

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
VLF Radio Detection of SIDs (Very low Frequency detection of Sudden Ionospheric Disturbances)

What balanced amplifiers could be used on a VLF loop antenna?

Admin May 25, 2026 No Comments

For a VLF loop antenna (typically covering a few kHz up to perhaps 30–300 kHz), a balanced amplifier should ideally have: Several approaches work well: Instrumentation Amplifiers These are often…

Radio observation in hydrogen line (1420MHz)

RF choke designs

Admin May 25, 2026 No Comments

An RF choke is an inductor designed to present a high impedance to radio-frequency currents while allowing DC or low-frequency currents to pass. The best design depends on the frequency…

VLF Radio Detection of SIDs (Very low Frequency detection of Sudden Ionospheric Disturbances)

HP10509A Circular Loop Antenna.

Admin May 25, 2026 No Comments

The HP 10509A Circular Loop Antenna is a specialized active magnetic-loop receiving antenna developed by Hewlett-Packard in the early 1960s. It was originally supplied with the HP 117A VLF Comparator…

Radio observation in hydrogen line (1420MHz)

What is a balanced feed line in radio astronomy?

Admin May 25, 2026 No Comments

A balanced feed line is a transmission line in which the two conductors carry equal currents in opposite directions, and neither conductor is connected to ground. The electromagnetic fields are…

VLF Radio Detection of SIDs (Very low Frequency detection of Sudden Ionospheric Disturbances)

Link for VLF meeting tonight

Admin May 25, 2026 No Comments

https://us06web.zoom.us/j/83880385896?pwd=RaJleLpl3wWahgD8q8JCFMbaybeg5N.1

Radio observation in hydrogen line (1420MHz) SETI Horn of Plenty (Hydrogen Line Pyramidal Horn Design Antenna)

What size oil tin about right to make WR650 waveguide for hydrogen line detection using a SETI Horn of Plenty?

Admin May 25, 2026 No Comments

For a WR-650 waveguide at the 1420 MHz hydrogen line, the internal dimensions need to be about 165 mm × 82.5 mm (6.5″ × 3.25″). That means you’re looking for…

Radio observation in hydrogen line (1420MHz) SETI Horn of Plenty (Hydrogen Line Pyramidal Horn Design Antenna)

Can pyramidal horn antennas be scaled by adding an extra bit on front?

Admin May 25, 2026 No Comments

Yes, a pyramidal horn antenna can generally be made larger by adding an additional flared section to the front, but there are some important caveats. A horn antenna works by…

Radio observation in hydrogen line (1420MHz)

I have a professionally made and sold 1420 MHz rectangular waveguide I purchased from ebay. The probe has a bulbous end which I understand widens the reception in some way. What is likely range of frequencies it can pick up?

Admin May 24, 2026 No Comments

If your 1420 MHz rectangular waveguide feed has a probe with a bulbous, paddle-shaped, or capacitive end, that feature is usually intended to broaden the impedance match rather than dramatically…

Radio observation in hydrogen line (1420MHz) SETI Horn of Plenty (Hydrogen Line Pyramidal Horn Design Antenna)

Horn antenna lecture from McMaster University

Admin May 24, 2026 No Comments

https://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L18_Horns.pdf

VLF Radio Detection of SIDs (Very low Frequency detection of Sudden Ionospheric Disturbances)

Painting the mount for the SETI Horn of Plenty at LRO 235/2026

Admin May 24, 2026 No Comments

Posts pagination

1 2 3 … 117

« Previous Page — Next Page »

Categories

  • ADVISORY NOTICE & DISCLAIMER
  • Aerials & Antennae
  • Airspy Software Defined Radios
  • Astronomy Art
  • Astronomy General Articles
  • Astrophotography
  • Attending & talking at conferences, workshops & societies
  • Aurorae Boreolis
  • BlurXterminator
  • Building radio telescopes
  • Cartoons
  • Cloud Chambers
  • Computer equipment for astronomy
  • Easy Radio Astronomy Software (ezRA)
  • Frequencies
  • Geoptik Nadirus 2BW Digital Setting Circles
  • GNU Radio
  • Hardware
  • International Space Station (ISS)
  • Introduction
  • JSol'Ex
  • Jupiter Radio Astronomy
  • KerberosSDR & Raspberry PI
  • Lichfield Radio Observatory (LRO) & its Equipment
  • Linux for Radio Astronomy
  • LRO-H1 Radio Telescope (86cm x 86cm Ptarmigan Triffid 4×4 Dipole Array)
  • LRO-H2 Radio Telescope (150cm Solar Cooker Dish)
  • LRO-H3 Radio Telescope (Alex Pettit H-Line Yagi)
  • Magnetometer
  • Making own Image Intensified Eyepieces
  • Maser Radio Observations
  • Meteor detection by radio
  • Michel Safir
  • Microscopy
  • Minolta AF 85mm F1.4 camera lens
  • MLAstro SHG 700 Spectroheliograph
  • Multimeters
  • Muon Detection
  • My interests in astronomy
  • NanoVNA
  • Night Sky Talks
  • Non-astronomy posts
  • Nooelec SAWBird LNAs
  • Observing Night Sky
  • Photography
  • PixInsight
  • Poetry & Songs
  • Pulsars
  • Radio Astronomy
  • Radio Interferometry
  • Radio observation in hydrogen line (1420MHz)
  • RTL-SDR Blog Software-Defined Radios (SDRs)
  • SARA
  • Science Fiction
  • SDRplay RSPduo Software-Defined Radio (SDR)
  • Seestar S50 Telescope
  • SETI Horn of Plenty (Hydrogen Line Pyramidal Horn Design Antenna)
  • Settings Radio Meteor Scatter Experiment
  • Software
  • Solar
  • Solar Cooker 1.5m Parabolic Dish Radio Telescope
  • Sony Alpha 7 Camera
  • Sony Alpha 99 Full-Frame Camera
  • Spectroscopy
  • Testing radio astronomy equipment
  • The 20 Metre Skynet Radio Dish at Green Bank Observatory
  • Thypoch Simera 35mm f/1.4 lens
  • Uncategorized
  • USRP B210 Software-Defined Radio
  • Videopad Software
  • VLF Radio Detection of SIDs (Very low Frequency detection of Sudden Ionospheric Disturbances)
  • Waveguides
  • Weather
  • Website management
  • Whisper Software
  • Windows
  • Wordpress

Recent Posts

  • Calculate for me, with downloadable sheet with equations as well, the practical maximum acceptable deviation in flare angle (give the actual angles too) of SETI Horn of Plenty with usual dimensions (give those) and with extension 1m in length on end.
  • Steps required to add Tensor Flow BXT to PixInsight – required by recent update
  • Maybe this is a stupid suggestion, but does all this mean that if users want the most accurate results they should keep their PicoMuon detectors in a fridge? And, if so, what would be the optimal temperature for the fridge to be set to?
  • Temperature response of UKRAA PicoMuon Muon Detector
  • The gain of a hydrogen horn or dish depends on its aperture which makes sense as bigger aperture means more light collected. But how does this work with a Yagi antenna tuned to hydrogen?

Recent Comments

  1. Admin on My 150cm LRO-H2 hydrogen line radio telescope is pointed azimuth 168 degrees, elevation 75 degrees, and collecting data by 24-hour transit scans. Which Milky Way parts does it pass through when trace shows one or two arms?
  2. Hugh Goodwin on My 150cm LRO-H2 hydrogen line radio telescope is pointed azimuth 168 degrees, elevation 75 degrees, and collecting data by 24-hour transit scans. Which Milky Way parts does it pass through when trace shows one or two arms?
  3. How to calculate a table showing attenuation of muons by lead thickness, and analysing the results I have obtained at LRO with difference quantities of lead between two CosmicWatch muon detectors in coincidence arrangement 17/5/2026 – astronomy.me.u on Calculating attenuation of muons in lead – ASCII text version
  4. Admin on My 150cm LRO-H2 hydrogen line radio telescope is pointed azimuth 168 degrees, elevation 75 degrees, and collecting data by 24-hour transit scans. Which Milky Way parts does it pass through when trace shows one or two arms?
  5. Jason Burnfield on Plots of data collected using Brian Coleman’s self-made hydrogen-line feed placed at correct (I think…but maybe not?) focal point on the LRO-H2 telescope (150cm Solar Cooker Radio Telescope) & pointed towards either outer Milky Way (1 spiral arm seen) or inner Milky Way (2 spiral arms seen) 16 May 2026

Archives

  • May 2026
  • April 2026
  • March 2026
  • February 2026
  • January 2026
  • December 2025
  • November 2025
  • October 2025
  • September 2025
  • August 2025
  • July 2025
  • June 2025
  • May 2025
  • April 2025
  • March 2025
  • February 2025
  • January 2025
  • December 2024
  • November 2024
  • October 2024
  • September 2024
  • August 2024
  • July 2024
  • June 2024
  • May 2024
  • April 2024
  • March 2024
  • February 2024
  • January 2024
  • December 2023
  • November 2023
  • October 2023
  • September 2023
  • June 2019
  • February 2019
  • April 2012

You missed

Uncategorized

Calculate for me, with downloadable sheet with equations as well, the practical maximum acceptable deviation in flare angle (give the actual angles too) of SETI Horn of Plenty with usual dimensions (give those) and with extension 1m in length on end.

PixInsight

Steps required to add Tensor Flow BXT to PixInsight – required by recent update

Muon Detection

Maybe this is a stupid suggestion, but does all this mean that if users want the most accurate results they should keep their PicoMuon detectors in a fridge? And, if so, what would be the optimal temperature for the fridge to be set to?

Muon Detection

Temperature response of UKRAA PicoMuon Muon Detector

All content is provided without any warranty of any kind. Use of the content of this website is entirely at your own risk, and we are not responsible for any injury or damage or loss of data or amenity arising from following advice in this website.

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

Astronomy observatory in Staffordshire, England.

Copyright © All rights reserved | Blogarise by Themeansar.