Cheapest way to make a new waveguide monopole
The waveguide in the centre of antennae sich as cantennae are made of a copper quarter wave monopole. The cheapest way to obtain a stiff enough short piece of copper…
The waveguide in the centre of antennae sich as cantennae are made of a copper quarter wave monopole. The cheapest way to obtain a stiff enough short piece of copper…
The following parameters allow ezCon to override the azimuth or elevation embedded within the data files from ezCol and use the parameter added to the ezCon command line instead: -ezConAzimuth…
This graph compares last week’s results with those found at a professional observatory in Finland (latter is neutron flux but gives basis for comparison as muons and neutrons go hand-in-hand).
See Powerpoint below: https://www.astronomy.me.uk/wp-content/uploads/2025/05/Comparison-data-collection-peaks-on-LRO-H2-and-LRO-H3-23-240525.pptx
The ideal thickness (gauge) of copper wire for the feed in a cantenna (typically for Wi-Fi at 2.4 GHz) depends on both practical and theoretical factors, mainly skin depth, mechanical…
I am running a NanoVNA workshop at EUCARA 2025 at Harwell Campus and as part of this I am going to demonstrate a mini-antenna testing range = I have been…
I have overlaid data from the SID Monitoring Station (purple) onto my data (red) on picture below (SID Monitoring Station A118 Home Page) Andy
Link below takes you to web-page where you can compare the hydrogen line spectra you have detected with your radio telescope with more professional results. Andy https://www.astro.uni-bonn.de/hisurvey/euhou/LABprofile
In September 2025, EUCARA is being held at Harwell Campus in UK. I am giving a talk and also running an introductory workshop on using NanoVNAs to test antennae/aerials. As…
Michiel kindly wrote this script for me to help me analyse the data I have from my Muon Detectors – these are the Cosmic Watch Muon Detectors – I have…