astronomy.network The Website of Lichfield Radio Observatory (LRO)

Modelling a 3 m dish at 1420.405 MHz in two ways: You’ll see: Diagrams: •           Unblocked beam 2D: •           Prime-focus

This comes up a lot in both radio astronomy and satellite communication when using prime-focus reflectors. On a prime-focus parabolic

There are several open-source software tools and libraries for interferometry / correlator / radio astronomy work. Depending on how much of

The “loss surface area” from a prime-focus feed is just the blocked (shadowed) aperture from the feed assembly (feed + support

The weight of a 6 ft × 4 ft sheet of plywood depends on its thickness and the wood species/density. Let’s go

Weight of a 5 ft × 5 ft sheet of fine aluminium window screening. Let’s work it out step by

Great 👍 let’s pin down what’s pulling in xterm. On Windows GNU Radio Companion (GRC), that usually comes from a

For a 30 cm jumper at 1420 MHz (H I line), RG174 and RG316 are effectively neck-and-neck—both cost you ~⅓–½ dB

That error message — “unable to scan ip19” — isn’t a standard GNU Radio error on its own. It usually comes from

That error message — “unable to scan ip19” — isn’t a standard GNU Radio error on its own. It usually comes from