6.3m Motorized Radio Telescope
Advanced Scientific System for Deep-Sky Radio Astronomy
Overview
The 6.3m Radio Telescope System is a high-performance instrument designed for
advanced research institutions, observatories, and
serious scientific programs.
With its large aperture and superior sensitivity, this system enables detection of
faint Hydrogen Line emissions, detailed galactic structures,
and weak deep-sky radio sources beyond the reach of smaller systems.
Key Features
- 6.3m Large Aperture Parabolic Dish for maximum signal capture
- High-Precision Alt/Azimuth Mount with continuous tracking accuracy
- Ultra-Low Noise Receiver Chain for faint signal detection
- Advanced Software For Radio Telescope Control And Data Analyze
- Multi-Band Expandable Architecture (future upgrades ready)
Typical Applications
- Deep Hydrogen Line Mapping – Milky Way structure and velocity fields
- Galactic Rotation Studies – Doppler shift measurements
- Solar Radio Monitoring – high-resolution burst analysis
- Weak Radio Source Detection – continuum observations
- University & Observatory Research Programs
Technology Overview
- High-precision parabolic reflector structure
- Robust tracking system for long-duration observations
- Low Noise Amplifier (LNA) optimized for weak signals
- Advanced digital signal processing and filtering
Software Platform
The system includes our Dynamic Planetarium Software, providing:
- Real-time sky visualization and telescope control
- FFT spectrum and high-resolution signal analysis
- Hydrogen Line scanning and Doppler shift measurement
- Scientific data export (CSV, FITS)
Software Interface
Push the Limits of Radio Astronomy
Maximum Sensitivity • Deep Sky Exploration • Observatory-Class Performance
