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Proceedings Paper

A dark-hole correction test for the step-transmission filter based coronagraphic system
Author(s): Jiangpei Dou; Deqing Ren; Yongtian Zhu; Xi Zhang; Rong Li
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Paper Abstract

We present the initial test of the dark-hole correction for the high-contrast imaging coronagraph that is based on the step-transmission filter. The dark hole is created by a 12x12 actuator deformable mirror (DM) that has been put in the conjugate plane of the pupil image of the coronagraph. In this test, we use the stochastic parallel gradient descent (SPGD) optimization algorithm to directly control the DM to provide an optimal phase to minimize the intensity in target regions, where the dark hole is created and the contrast can be enhanced. For demonstration purpose, the test is carried out in a single wavelength and should be improved in next step for broad-band high-contrast imaging. Finally, it is shown in the test that an extra contrast ~50 times improvement has reached in the dark hole in the coronagraphic image plane. Such a technique could be used for a future space-based high-contrast observation and is promising for the direct imaging of an Earth-like exoplanet.

Paper Details

Date Published: 21 September 2012
PDF: 7 pages
Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84420D (21 September 2012); doi: 10.1117/12.924248
Show Author Affiliations
Jiangpei Dou, Nanjing Institute of Astronomical Optics & Technology (China)
Deqing Ren, Nanjing Institute of Astronomical Optics & Technology (China)
California State Univ., Northridge (United States)
Yongtian Zhu, Nanjing Institute of Astronomical Optics & Technology (China)
Xi Zhang, Nanjing Institute of Astronomical Optics & Technology (China)
Graduate Univ. of the Chinese Academy of Sciences (China)
Rong Li, Nanjing Institute of Astronomical Optics & Technology (China)
Graduate Univ. of the Chinese Academy of Sciences (China)


Published in SPIE Proceedings Vol. 8442:
Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave
Mark C. Clampin; Giovanni G. Fazio; Howard A. MacEwen; Jacobus M. Oschmann, Editor(s)

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