Lucky Imaging
The foundation of planetary photography - selecting only the sharpest frames from thousands captured to overcome atmospheric turbulence
How It Works
Capture high-speed video at 60-200 fps to freeze atmospheric turbulence
Software calculates D/r0 ratio (telescope aperture vs Fried parameter) to determine selection rate
Frame quality is measured using Laplacian variance or similar sharpness metrics
Typical selection: 1-10% for poor seeing, 10-30% average, 30-50% good, 50%+ excellent
At 1% selection rate, amateur telescopes can approach diffraction-limited resolution (Strehl ratio >0.8)
Selected frames are aligned using centroid or multi-point registration
Stacking averages out remaining noise while preserving sharp detail
Pro Tips
- -The D/r0 ratio determines optimal selection: larger aperture needs stricter selection in average seeing
- -Pickering 7-8 seeing allows 30-50% stacking; Pickering 4-5 may need only 5-10%
- -Capture 5000+ frames minimum - more frames = better selection pool
- -ROI (640x480) can achieve 200+ fps vs 30fps full-frame - crucial for lucky imaging
- -Short exposures (5-20ms) freeze seeing better than long exposures
Related Algorithms
Related Terms
Seeing
Atmospheric turbulence affecting image sharpness
Stacking
Combining multiple frames into a single high-quality image
Frame Rate (FPS)
Number of frames captured per second
ROI (Region of Interest)
Cropping the sensor to increase frame rate
Seeing Scale (Pickering/Antoniadi)
Numerical rating of atmospheric stability for planning captures
Try Lucky Imaging
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