Paper
12 October 2004 High-contrast imaging testbed for the Terrestrial Planet Finder coronagraph
Author Affiliations +
Abstract
The Terrestrial Planet Finder (TPF) mission is planning to launch a visible coronagraphic space telescope in 2014. To achieve TPF science goals, the coronagraph must have extreme levels of wavefront correction (less than 1 Å rms over controllable spatial frequencies) and stability to get the necessary suppression of diffracted starlight (~1E-10 contrast at an angular separation ~4 lambda/D). TPF Coronagraph’s primary platform for experimentation is the High Contrast Imaging Testbed, which will provide laboratory validation of key technologies as well as demonstration of a flight-traceable approach to implementation. Precision wavefront control in the testbed is provided by a high actuator density deformable mirror. Diffracted light control is achieved through use of occulting or apodizing masks and stops. Contrast measurements will establish the technical feasibility of TPF requirements, while model and error budget validation will demonstrate implementation viability. This paper describes the current testbed design, development approach, and recent experimental results.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrew E. Lowman, John T. Trauger, Brian Gordon, Joseph Jacob Green, Dwight Moody, Albert F. Niessner, and Fang Shi "High-contrast imaging testbed for the Terrestrial Planet Finder coronagraph", Proc. SPIE 5487, Optical, Infrared, and Millimeter Space Telescopes, (12 October 2004); https://doi.org/10.1117/12.547710
Lens.org Logo
CITATIONS
Cited by 20 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Coronagraphy

Cameras

Mirrors

Planets

Wavefront sensors

Wavefronts

Control systems

RELATED CONTENT

EXCEDE technology development III: first vacuum tests
Proceedings of SPIE (August 02 2014)
Wavefront control in space with MEMS deformable mirrors
Proceedings of SPIE (March 05 2013)
Pupil mapping Exoplanet Coronagraphic Observer (PECO)
Proceedings of SPIE (July 12 2008)
TPF-C: status and recent progress
Proceedings of SPIE (June 27 2006)
Eclipse architecture
Proceedings of SPIE (March 03 2003)

Back to Top