Block diagram of hydrogen line (1420 MHz) radio telescope
I prepared this diagram of 1420 MHz telescope. Andy
I prepared this diagram of 1420 MHz telescope. Andy
There have been many expert and knowledgeable comments about cantenna feed design on this group and on the SARA RTOP yesterday by people who truly understand the subject – we…
Website recommended by Alex Pettit: https://www.changpuak.ch/electronics/cantenna.php
To design an effective waveguide for 1420 MHz (21 cm hydrogen line), you need to consider several factors, including waveguide dimensions, material, and feed design. Here’s a step-by-step guide to…
Click 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 data files https://www.astronomy.me.uk/wp-content/uploads/2025/01/LRO-H2SCRT_Integ1100000_250128.zip Results of processing data in ezCon scipt…
This shows the repeated patterns of data emerging from the drift scans of LRO-H1(Ptarmigan) hydrogen line radio telescope at LRO & the generation of contour maps using Rinearn3D. The use…
LRO-H3 1420MHz tuned aerial (Alex Pettit Plate Yagi) not showing difference between sky and ground. Why might this be? Handmade tuned 1420MHz with 13 elements and RTL-SDR Blog V3 software…
This 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 52.7 -ezRAObsLon -1.8 -ezRAObsAmsl 81.0 -ezRAObsName LRO-H1(Ptarmigan)ezCol_1400-27MCav+SAWB_LMR400_FreqRef_1422-405_Bandwidth_1-000_El-40-1_Az_163 -ezColAzimuth 163 -ezColElevation…
Detecting the hydrogen line at 1420.4058 MHz is a popular project among amateur radio astronomers, and several software-defined radios (SDRs) are suitable for this purpose when paired with appropriate antennas…
Detecting the 21 cm hydrogen line (the characteristic emission from neutral hydrogen in the Milky Way) requires a radio antenna sensitive to that wavelength. The wavelength of this emission is…