5.3m Motorized Radio Telescope
Research-Grade System for Advanced Radio Astronomy
Overview
The 5.3m Radio Telescope System is designed for serious scientific applications,
universities, and research institutions requiring high sensitivity and
enhanced angular resolution.
With its larger aperture, the system enables precise observation of the
21 cm Hydrogen Line, detailed solar radio emissions, and
weak galactic and extragalactic radio sources.
Key Features
- 5.3m High-Gain Parabolic Dish for maximum signal collection
- Precision Alt/Azimuth GoTo Mount with continuous tracking
- High-Sensitivity Receiver Chain for weak signal detection
- Advanced Software For analyzing Radio Data and Controlling Radio Telescope
- Expandable Multi-Frequency Capability
Typical Applications
- Hydrogen Line Surveys – detailed galactic structure mapping
- Solar Radio Astronomy – monitoring flares and bursts
- Deep Sky Radio Sources – continuum measurements
- Scientific Research Projects
Technology Overview
- High-performance parabolic reflector
- Precision tracking system
- Low Noise Amplifier (LNA)
- Advanced digital signal processing
Software Platform
The system includes our Dynamic Planetarium Software, providing:
- Real-time sky visualization and tracking
- FFT spectrum and radio signal analysis
- Hydrogen Line scanning and visualization
- Scientific data export (CSV, FITS)
Software Interface
Step Into Professional Radio Astronomy
High Sensitivity • Deep Sky Access • Research-Grade Performance
