Laboratory demonstration of a focal plane coronagraphic interferometer designed for anti-halo apodization of starlight

Nicole Putnam, Johanan L. Codona, J Roger P Angel

Research output: Chapter in Book/Report/Conference proceedingConference contribution

9 Citations (Scopus)

Abstract

The coronagraphic focal plane interferometer reflects away the core starlight with a mirror in the focal plane and uses it to form a coherent interferometric reference beam. This is used in a Mach-Zehnder configuration with phase shifting to measure the complex amplitude of the star halo speckles in the focal plane where the interference takes place. We present results from a laboratory prototype in which the speckles are suppressed over half the field by modifying the waverront in a pupil plane with a MEMS deformable mirror, based on a Fourier transform of the complex halo derived from the focal plane interferometric data. Even deeper suppression of the residual stellar halo over the full 360 degree field will be possible by explicitly constructing an "anti-halo" from the reference beam; a new technique for exoplanet imaging (Codona and Angel, 2004). We present the design and current status of a laboratory prototype to study antihalo apodization. The spatially-filtered core starlight will be modulated by deformable mirrors in a Michelson configuration to form a temporally-coherent copy of the measured residual complex halo, with the same amplitude but opposite phase (i.e. an "anti-halo"). Using components with only modest control accuracy, the method has the potential to reduce an already low residual halo by an additional two decades.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
Volume6272 II
DOIs
StatePublished - 2006
EventAdvances in Adaptive Optics II - Orlando, FL, United States
Duration: May 24 2006May 31 2006

Other

OtherAdvances in Adaptive Optics II
CountryUnited States
CityOrlando, FL
Period5/24/065/31/06

Fingerprint

apodization
Speckle
Interferometers
halos
Mirrors
Demonstrations
interferometers
Mach number
Stars
MEMS
Fourier transforms
Imaging techniques
deformable mirrors
prototypes
extrasolar planets
pupils
configurations
microelectromechanical systems
retarding
mirrors

Keywords

  • Coronagraph
  • Extreme Adaptive Optics
  • Focal Plane
  • Interferometer

ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Condensed Matter Physics

Cite this

Putnam, N., Codona, J. L., & Angel, J. R. P. (2006). Laboratory demonstration of a focal plane coronagraphic interferometer designed for anti-halo apodization of starlight. In Proceedings of SPIE - The International Society for Optical Engineering (Vol. 6272 II). [62722M] https://doi.org/10.1117/12.672723

Laboratory demonstration of a focal plane coronagraphic interferometer designed for anti-halo apodization of starlight. / Putnam, Nicole; Codona, Johanan L.; Angel, J Roger P.

Proceedings of SPIE - The International Society for Optical Engineering. Vol. 6272 II 2006. 62722M.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Putnam, N, Codona, JL & Angel, JRP 2006, Laboratory demonstration of a focal plane coronagraphic interferometer designed for anti-halo apodization of starlight. in Proceedings of SPIE - The International Society for Optical Engineering. vol. 6272 II, 62722M, Advances in Adaptive Optics II, Orlando, FL, United States, 5/24/06. https://doi.org/10.1117/12.672723
Putnam N, Codona JL, Angel JRP. Laboratory demonstration of a focal plane coronagraphic interferometer designed for anti-halo apodization of starlight. In Proceedings of SPIE - The International Society for Optical Engineering. Vol. 6272 II. 2006. 62722M https://doi.org/10.1117/12.672723
Putnam, Nicole ; Codona, Johanan L. ; Angel, J Roger P. / Laboratory demonstration of a focal plane coronagraphic interferometer designed for anti-halo apodization of starlight. Proceedings of SPIE - The International Society for Optical Engineering. Vol. 6272 II 2006.
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