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Image Restoration in Strong Atmospheric Turbulence

Trent Kyono Institute for Astronomy Mentor: Douglas Hope. Image Restoration in Strong Atmospheric Turbulence. How to Model a Point Spread Function (PSF). Point Source. Wave-front (planar). Phase. Atmosphere (no turbulence). Turbulence Layer in Atmosphere. PSF.

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206 views • 19 slides

How to start (initial training)

How to start (initial training). FLL July 2011. Training preparation. Customer to provide team list with r esponsibility of team members (admin, tech etc.) c omputer knowledge of team members

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232 views • 12 slides

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Ifa staff - PowerPoint PPT Presentation

Image Restoration in Strong Atmospheric Turbulence

How to start (initial training)