Paper
6 August 2014 A coronagraph based on two spatial light modulators for active amplitude apodizing and phase corrections
Jiangpei Dou, Deqing Ren, Xi Zhang, Yongtian Zhu, Gang Zhao, Zhen Wu, Rui Chen, Chengchao Liu, Feng Yang, Chao Yang
Author Affiliations +
Abstract
Almost all high-contrast imaging coronagraphs proposed until now are based on passive coronagraph optical components. Recently, Ren and Zhu proposed for the first time a coronagraph that integrates a liquid crystal array (LCA) for the active pupil apodizing and a deformable mirror (DM) for the phase corrections. Here, for demonstration purpose, we present the initial test result of a coronagraphic system that is based on two liquid crystal spatial light modulators (SLM). In the system, one SLM is served as active pupil apodizing and amplitude correction to suppress the diffraction light; another SLM is used to correct the speckle noise that is caused by the wave-front distortions. In this way, both amplitude and phase error can be actively and efficiently compensated. In the test, we use the stochastic parallel gradient descent (SPGD) algorithm to control two SLMs, which is based on the point spread function (PSF) sensing and evaluation and optimized for a maximum contrast in the discovery area. Finally, it has demonstrated a contrast of 10-6 at an inner working angular distance of ~6.2 λ/D, which is a promising technique to be used for the direct imaging of young exoplanets on ground-based telescopes.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jiangpei Dou, Deqing Ren, Xi Zhang, Yongtian Zhu, Gang Zhao, Zhen Wu, Rui Chen, Chengchao Liu, Feng Yang, and Chao Yang "A coronagraph based on two spatial light modulators for active amplitude apodizing and phase corrections", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91478O (6 August 2014); https://doi.org/10.1117/12.2055327
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Cited by 1 scholarly publication.
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KEYWORDS
Spatial light modulators

Coronagraphy

Point spread functions

Exoplanets

Imaging systems

Telescopes

Phase shift keying

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