Phase and amplitude control ability using spatial light modulators and zero length difference Michelson interferometer

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 4854, Issue , 2002, Pages 405-412

  Littman, Michael G ^a   Carr, Michael ^a   Leighton, Jim ^a   Burke, Ezekiel ^a   Spergel, David ^b   Kasdin, Jeremy ^a  

^a Princeton University   (United States)

^b PRINCETON UNIVERSITY   (United States)

Author keywords

Amplitude correction; Michelson interferometer; Phase correction; Spatial light modulator; White light

Indexed keywords

ASTROPHYSICS; GALAXIES; HELIUM NEON LASERS; INTERFEROMETERS; LIGHT MEASUREMENT; LIGHT MODULATORS; LIQUID CRYSTALS; MIRRORS; OPTICAL VARIABLES CONTROL; PLANETS; SPACE TELESCOPES;

AMPLITUDE CORRECTION; MICHELSON INTERFEROMETER; PHASE CORRECTION; WHITE LIGHT;

IMAGING TECHNIQUES;

EID: 0038532313     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.459813     Document Type: Conference Paper

References (2)

1. For an early report of the Spergel Pupil see: M.G. Littman, J. Kasdin, and D. Spergel, "A Gaussian Pupil Coronagraph: A New Approach to Detecting Terrestrial Planets", American Astronomical Society Annual Meeting (Pasadena, CA), June 3-7 (2001).
2. R. Dou and M.K. Giles, "Closed Loop Adaptive Optics System using a LCTV as a Phase Retarder" Opt. Lett 20, 1583 (1995).