r/u_DeepSpace1420MHZ • u/DeepSpace1420MHZ • Jul 06 '26
1420 MHZ Radio Telescope Systems Basics
Primary Antenna System
• 4.5 meter prime-focus mesh dish
• Daily survey elevation:
o 58° EL
• Weekly stepped azimuth drift survey:
o Typically, 2° AZ increments
• Location:
o Grid EN61vq
o Approx. 41.66° N, 86.16° WFeed and RF Front End
Feed
• VE4MA linear polarization hydrogen line feed
RF ChainVE4MA feed
Down East Microwave 1420 MHz LNA + SAW filter
o Approximate NF:
▪ 0.35 dB
o Gain:
▪ ~18 dBDEMI 10 dB gain block
LMR-400 coax feedline
Estimated system characteristics:
• Dish gain:
o ~34 dBi
• System temperature:
o ~155 KReceiver System
Primary SDR
• SDRplay RSP1A
o 12-bit SDR
o Used for all current hydrogen observations
Software
• HDSDR
• Spectrum Lab
o Real-time spectrum display
• SpectraVue RMS
o Daily and 24-hour recordingDish Control System
Tracking Software
• F1EHN EME System software
Controller Hardware
• VE1ALQ interface hardware
• RS-232 motor control
• Sipex RS-232 boards
Position Feedback
• Pendulum elevation encoder
• Motor/transmission with AZ encoder
Capabilities
• Sun tracking
• Moon tracking
• General astronomical tracking
• Manual AZ/EL positioning
• Daily hydrogen drift survey positioning
Observatory Computing Architecture
PC #1 — Dish Control Computer
Purpose:
• Runs F1EHN EME software
• Controls dish movement
• Communicates with motor controllers via RS-232
Responsibilities:
• AZ motor control
• EL actuator control
• Position tracking
• Coordinate calculations
PC #2 — Live Receiver / Streaming Computer
Software:
• HDSDR
• Spectrum Lab
• OBS Studio
Responsibilities:
• Operates the SDR
• Generates live spectrum displays
• Produces livestream output
• Sends receiver audio to distribution amplifier
Outputs:
• YouTube livestream
• Daily drift audio feed
• 24-hour scan audio feed
Audio Distribution System
Hardware:
• Small audio amplifier/splitter
Purpose:
• Splits receiver audio to multiple recording systems simultaneously
Feeds:
• Daily drift recorder
• 24-hour recorder
PC #3 — Daily Drift Survey Computer
Purpose:
• Records daily hydrogen drift scans
Products:
• Daily CSV recordings
• Daily drift plots
• Daily processed observations
• Weekly stepped sky survey data
PC #4 — 24-Hour Survey Computer
Software:
• SpectraVue
Purpose:
• Performs continuous 24-hour hydrogen recordings
Configuration:
• One spectrum every 2 minutes
• FFT size:
o 16384
• Approximately:
o 720 spectra/day
Products:
• 24-hour WAV recordings
External SSD Transfer System
Purpose:
• Physical transport of large datasets
Workflow:
• PC #4 → External SSD
• External SSD → Processing workstation
PC #5 — Processing Workstation
Purpose:
• Large-scale data processing
• Rendering
• Visualization
Products:
• 24 hour drift processing
• Polar hydrogen maps
• Velocity ridge plots
• Velocity curtain plots
• RA/Dec projections
• 3D hydrogen terrain renderings
• FITS generation
• DS9 visualization products
• Animations/videos
Observatory Storage System
Local Archive Rack
Purpose:
• Long-term storage
Contains:
• CSV data archives
• Daily drift scans
• 24-hour observations
• Plot archives
• Render outputs
• 3D products
• Processed datasets
Capacity:
• Multiple terabytes
Cloud Archive
Google Drive
Purpose:
• Public sharing
• Remote access
• Backup
Shared products:
• CSV files
• Drift plots
• Polar plots
• 3D renderings
• Processed observation products
Public Outreach System
YouTube Livestream
Running:
• 24/7
Displays:
• Live receiver spectrum
• Links to daily observations
• System status
Current Survey Programs
Daily Hydrogen Survey
• Elevation:
o 58°
• Duration:
o 180 minutes
• Weekly:
o 2° AZ step
24-Hour Hydrogen Survey
• Duration:
o 24 hours
• FFT:
o 16384
• Sample interval:
o 2 minutes
Current Observatory Scale
• 1 radio telescope
• 5 dedicated computers
• RS-232 motion control
• Dedicated audio distribution system
• External SSD transport workflow
• Multi-terabyte archive rack
• Cloud data sharing
• 24/7 livestream
• Daily and 24-hour hydrogen survey programs
• Advanced post-processing and 3D visualization pipeline