Link for VLF meeting tonight
https://us06web.zoom.us/j/83880385896?pwd=RaJleLpl3wWahgD8q8JCFMbaybeg5N.1
https://us06web.zoom.us/j/83880385896?pwd=RaJleLpl3wWahgD8q8JCFMbaybeg5N.1
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…
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…
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…
https://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L18_Horns.pdf
A perk of SARA membership that we can use the 20m Skynet dish. The angular size of the Andromeda Galaxy (M31) depends on how faint an outer region you include:…
Using medium-format lenses on a full-frame A-mount body like the Sony Alpha A99 is a niche but very enjoyable setup if you like manual focus, unusual rendering, and superb central…
For two identical horizontal scintillators of size 5 x 5 cm, the coincidence rate drops as detector spacing increases because the allowed angular acceptance narrows. A useful estimate is: tan(theta_max)…
Yes — there have been a few measurements and discussions of temperature effects in CosmicWatch-style scintillator/SiPM muon detectors, though not many formal dedicated studies. The main effect is usually not…