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Lucky Imaging

The foundation of planetary photography - selecting only the sharpest frames from thousands captured to overcome atmospheric turbulence

How It Works

1

Capture high-speed video at 60-200 fps to freeze atmospheric turbulence

2

Software calculates D/r0 ratio (telescope aperture vs Fried parameter) to determine selection rate

3

Frame quality is measured using Laplacian variance or similar sharpness metrics

4

Typical selection: 1-10% for poor seeing, 10-30% average, 30-50% good, 50%+ excellent

5

At 1% selection rate, amateur telescopes can approach diffraction-limited resolution (Strehl ratio >0.8)

6

Selected frames are aligned using centroid or multi-point registration

7

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

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