3.7m Motorized Radio Telescope
High Performance System for Advanced Radio Astronomy
Overview
The 3.7m Radio Telescope System is designed for advanced amateur astronomers,
universities, and research institutions seeking higher sensitivity and improved angular resolution.
With its larger aperture and precision mechanics, this system enables detailed observation of the
21 cm Hydrogen Line, solar radio emissions, and
deep-sky radio sources.
Key Features
- 3.7m High-Precision Dish with optimized surface accuracy
- Alt/Azimuth GoTo Mount with real-time celestial tracking
- High Sensitivity Receiver Chain for weak signal detection
- Complete Software Package For Radio Data Analyze And Radio Telescope Control
- Expandable Architecture for multi-frequency observations
Typical Applications
- Hydrogen Line Mapping – study galactic structure
- Solar Radio Monitoring – detect flares and bursts
- Continuum Observations – measure radio sources
- Educational & Research Use
Performance Upgrade vs 3.0m
| Parameter | 3.0m | 3.7m |
|---|---|---|
| Sensitivity | Standard | +50% Improvement |
| Resolution | Moderate | Higher Angular Resolution |
| Applications | Educational | Research Capable |
Technology Overview
- High-performance parabolic reflector
- Precision tracking system
- Low Noise Amplifier (LNA)
- Digital signal processing
Software Platform
The system includes our Dynamic Planetarium Software, providing:
- Real-time sky visualization
- FFT spectrum analysis
- Hydrogen Line scanning
- Data export (CSV, FITS)
Software Interface
Upgrade Your Radio Astronomy Capabilities
Higher Sensitivity • Better Resolution • Research Ready
