Abstract

In the high photon flux limit a diffraction-limited picture of an astronomical object may be recovered from a single turbulence-degraded image. The method proposed is based upon a simple extension of the phase closure method and requires the use of a specially designed interferometer.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.