Two-camera wavefront estimation with a Gercheberg-Saxton based scheme

Most mature wavefront-estimation algorithms for high-contrast imaging rely on a-priori knowledge of the deformable mirror (DM) surface and thus are limited by uncertainty in the physics of the DM. In this paper, we review the DM diversity wavefront estimation algorithm and introduce a DM-independent method of wavefront estimation that utilizes two cameras and a Gerchberg-Saxton-based iterative phase retrieval scheme. We compare the two estimation algorithms, and we present the creation of a dark hole in the image plane using the Stroke Minimization correction algorithm and this two-camera estimation.

[1]  Amir Give'on,et al.  Broadband wavefront correction algorithm for high-contrast imaging systems , 2007, SPIE Optical Engineering + Applications.

[2]  Jason David Kay Electric field estimation for high-contrast imaging , 2009 .

[3]  R. Vanderbei,et al.  Spiderweb Masks for High-Contrast Imaging , 2003, astro-ph/0303049.

[4]  J. Green,et al.  Reflectivity and optical surface height requirements in a broadband coronagraph. 1. Contrast floor due to controllable spatial frequencies. , 2006, Applied optics.

[5]  R. Gerchberg A practical algorithm for the determination of phase from image and diffraction plane pictures , 1972 .

[6]  Ruslan Belikov,et al.  Wavefront correction in a shaped-pupil coronagraph using a Gerchberg-Saxton-based estimation scheme , 2007, SPIE Optical Engineering + Applications.

[7]  Marc J. Kuchner,et al.  EIGHTH-ORDER IMAGE MASKS FOR TERRESTRIAL PLANET FINDING , 2005 .

[8]  J R Fienup,et al.  Phase retrieval algorithms: a comparison. , 1982, Applied optics.

[9]  N Jeremy Kasdin,et al.  Optimal one-dimensional apodizations and shaped pupils for planet finding coronagraphy. , 2005, Applied optics.

[10]  R. Vanderbei,et al.  Rectangular-Mask Coronagraphs for High-Contrast Imaging , 2004, astro-ph/0401644.

[11]  R. Vanderbei,et al.  Extrasolar Planet Finding via Optimal Apodized-Pupil and Shaped-Pupil Coronagraphs , 2003 .

[12]  Robert J. Vanderbei,et al.  Extrasolar Planet Finding via Optimal Apodized and Shaped Pupil , 2002 .

[13]  Benjamin F. Lane,et al.  Planet detection in visible light with a single aperture telescope and nulling coronagraph , 2002, SPIE Optics + Photonics.

[14]  Laurent Pueyo Broadband contrast for exo -planet imaging: The impact of propagation effects , 2008 .

[15]  R. Vanderbei,et al.  Circularly Symmetric Apodization via Star-shaped Masks , 2003, astro-ph/0305045.

[16]  J. H. Seldin,et al.  Numerical investigation of the uniqueness of phase retrieval , 1990 .

[17]  S. Ridgway,et al.  Exoplanet Imaging with a Phase-induced Amplitude Apodization Coronagraph. III. Diffraction Effects and Coronagraph Design , 2006 .

[18]  L. Pueyo,et al.  Optimal dark hole generation via two deformable mirrors with stroke minimization. , 2009, Applied optics.

[19]  S. Ridgway,et al.  Exoplanet Imaging with a Phase-induced Amplitude Apodization Coronagraph. I. Principle , 2004, astro-ph/0412179.