GNU Radio Glowgraph on dedispersion
📡 GNU Radio Dedispersion Flowgraph (ASCII) 🧠 Dedispersion Core Idea (ASCII) Dispersion delay: Convert to samples: Each channel is delayed differently, then aligned and summed. 🧩 Key Block Notes Signal…
📡 GNU Radio Dedispersion Flowgraph (ASCII) 🧠 Dedispersion Core Idea (ASCII) Dispersion delay: Convert to samples: Each channel is delayed differently, then aligned and summed. 🧩 Key Block Notes Signal…
Dedispersion is a signal-processing technique used in radio astronomy to correct for the effect of interstellar dispersion—the way radio waves get “smeared out” as they travel through space. 🌌 What…
Hi Andrew I have attached two files (accessible via link at bottom of this post), which need to be copied onto the RPi. I have changed their names because a…
Got it — you mean the next size up from the Yaesu G-5500DC antenna rotator. Short answer: there is no direct “next model up” that is the same type. Moving…
The Yaesu G-5500DC doesn’t have a single simple “load capacity” like a crane or mount — Yaesu specifies it using several related limits. The key figures are: ✅ Primary load…
Short answer: there’s no clearly published “official” payload figure for the TV1 Minimaster mount itself—but you can still estimate it fairly reliably from comparable hardware and its intended use. What…
Yes — but there’s an important distinction that matters for your use case: 👉 Most cheap USB inclinometer devices are USB-rechargeable only (power),👉 Very few actually output angle data over…
Yes — there are self-contained telescope pointing systems, but they come in a few different flavours depending on how “universal” and “self-contained” you want. The key term to look for…
At 20 kHz you’re really designing a resonant system, not just adding a tuner box. For your kind of radio astronomy / interferometry work, the most practical approach is a…
From Brian Coleman: Hello Andrew, Looking at your photo the feed looks much too close to the dish. You need to calculate the focus point of the dish. The phase…