How to design an effective 1420 MHz waveguide from ChatGPT
To design an effective waveguide for 1420 MHz (21 cm hydrogen line), you need to consider several factors, including waveguide
Read moreAndrew Thornett, Lichfield, England, M6THO, andrew (at) thornett (dot) net
To design an effective waveguide for 1420 MHz (21 cm hydrogen line), you need to consider several factors, including waveguide
Read moreClick on links below to download data: ezCol .txt data files https://www.astronomy.me.uk/wp-content/uploads/2025/01/data-300125.zip SDR Sharp data generated from conversion of above
Read moreThis shows the repeated patterns of data emerging from the drift scans of LRO-H1(Ptarmigan) hydrogen line radio telescope at LRO
Read moreLRO-H3 1420MHz tuned aerial (Alex Pettit Plate Yagi) not showing difference between sky and ground. Why might this be? Handmade
Read moreThis is the current batch file used with LRO-H1: REM NORMAL RESOLUTION (IE STANDARD SETTINGS) cd C:\cd C:\Data\ezRA_Program+Data\LRO\py ..\ezRA\ezCol.py -ezRAObsLat
Read moreClick on links to download the workflow: Workflow (PDF) – https://www.astronomy.me.uk/wp-content/uploads/2025/01/Andrew-Thornett-Astrophoto-Processing-Workflow-220125.pdf Workflow (.docx file) – https://www.astronomy.me.uk/wp-content/uploads/2025/01/Andrew-Thornett-Astrophoto-Processing-Workflow-220125.docx
Read moreThis list needs to be added to the repository list within PixInsight: https://raw.githubusercontent.com/setiastro/pixinsight-updates/main https://www.rc-astro.com/BlurXTerminator/PixInsight https://www.rc-astro.com/NoiseXTerminator/PixInsight https://www.rc-astro.com/StarXTerminator/PixInsight https://www.rc-astro.com/TensorFlow/PixInsight/CPU https://pixinsight.astroprocessing.com https://www.ghsastro.co.uk/updates https://www.ideviceapps.de/PixInsight/Utilities
Read moreLocated at: C:\Users\andre\AppData\Roaming\Pleiades
Read moreDetecting the hydrogen line at 1420.4058 MHz is a popular project among amateur radio astronomers, and several software-defined radios (SDRs)
Read moreDetecting the 21 cm hydrogen line (the characteristic emission from neutral hydrogen in the Milky Way) requires a radio antenna
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