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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.

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Easy Radio Astronomy Software (ezRA)

How to use GLon.py in ezRA (Easy Radio Astronomy)

Admin January 23, 2026 No Comments

ezRA’s ezGLon.py program studies cross sections of the Milky Way, along one Galactic Longitude (GLon). ezRA’s ezGLon.py program processes *GLon.npz files. Above, the ezGLon.py program errored because it found *Gal.npz…

Easy Radio Astronomy Software (ezRA) LRO-H2 Radio Telescope (150cm Solar Cooker Dish) Radio observation in hydrogen line (1420MHz)

Hydrogen Line peak (H-Line, 1420 MHz) screen capture from ezCol.py capture software (part of ezRA suite) collecting data from a RTL-SDR Blog v3 Software Defined Radio on LRO-H2 radio telescope (150cm dish) on 22/1/2026

Admin January 22, 2026 No Comments
Radio observation in hydrogen line (1420MHz)

What is the impedance of 1420 Mhz (1.42 GHz) [atomic neutral hydrogen line] dipole?

Admin January 21, 2026 No Comments

A half-wave dipole resonant at 1420 MHz (the hydrogen line) has essentially the same impedance as at any other frequency: In practice The actual feedpoint impedance will vary depending on…

Radio observation in hydrogen line (1420MHz)

When I observe Milky Way in hydrogen, the centre of the galaxy has little hydrogen line emission. Why is that?

Admin January 21, 2026 No Comments

What you’re seeing is real, and it surprises a lot of people the first time they map the Galaxy in the 21-cm line. In short: the Galactic centre is not…

Radio observation in hydrogen line (1420MHz)

When I detect hydrogen with my radio telescope, is it coming from the optically bright spiral arms or the optically dark areas between them?

Admin January 21, 2026 No Comments

Mostly from the optically dark regions between the spiral arms, not from the bright arms themselves. Here’s why that happens, and how it matches what you’re detecting. 1. What the…

Radio observation in hydrogen line (1420MHz)

1-4GHz Loop Feed fabrication (Alex Pettit)

Admin January 21, 2026 No Comments
Radio observation in hydrogen line (1420MHz)

Calculating the length of 1.4GHz Hydrogen Monopole Probe to use inside a cantenna

Admin January 21, 2026 No Comments

Posted by Alex Pettit on SARA Mailing List 18/1/2026: Typical calculation for a one quarter wavelength (1/4 WL) antenna is WL / 4 * 0.95 211 /4 * 0.95 =…

Radio observation in hydrogen line (1420MHz)

Incorrect length of boom for feed on Nooelec 1.4 GHz tuned mesh dish and feed

Admin January 21, 2026 No Comments

Following results of investigations by Alex Pettit were posted on SARA Mailing List 20/1/2026: The “Nooelec 1.4GHz” feed seems improperly designed : the Focal Point of a 1m f/D 0.35…

Radio observation in hydrogen line (1420MHz)

Wavelength observed in hydrogen line radio astronomy

Admin January 20, 2026 No Comments
Jupiter Radio Astronomy

Wavelength observed by RADIO JOVE

Admin January 20, 2026 No Comments

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Recent Posts

  • If I want to make a bigger version of the SETI Horn of Plenty, still for 1420 MHz, how do I increase the dimensions?
  • How does flared section of hydrogen line horn antenna scale with changes in wavelength measured?
  • Find me an URL for original SETI Horn of Plenty dimensions
  • Data .txt Files & Timelapse Video of Data Collection of comparison between ezCol.py & ezColGR (GNU Radio version) on LRO-H2(SCRT) using same 150cm dish, feed and SDR 24-25/1/2026
  • Data Collection Videos from LRO-H1(Ptarmigan Array) 23-24/1/2026 with use of ezColGR test GNU Radio Script

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  1. Yoshiyuki Takeyasu on What is a geodesic parabolic dish?
  2. Admin on What is a geodesic parabolic dish?
  3. Yoshiyuki Takeyasu on What is a geodesic parabolic dish?
  4. Stephen Arbogast on Designing tuneable LRO aluminium stove pipe cantenna H-Line 16/1/2025
  5. Yoshiyuki Takeyasu on What is a geodesic parabolic dish?

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You missed

Uncategorized

If I want to make a bigger version of the SETI Horn of Plenty, still for 1420 MHz, how do I increase the dimensions?

Uncategorized

How does flared section of hydrogen line horn antenna scale with changes in wavelength measured?

Uncategorized

Find me an URL for original SETI Horn of Plenty dimensions

Uncategorized

Data .txt Files & Timelapse Video of Data Collection of comparison between ezCol.py & ezColGR (GNU Radio version) on LRO-H2(SCRT) using same 150cm dish, feed and SDR 24-25/1/2026

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Astronomy observatory in Staffordshire, England.

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