Paper
25 August 2009 Stellar coronagraph performance impact due to particulate contamination and scatter
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Abstract
The detection and characterization of earth-like exo-planets with space coronagraph instruments could be adversely affected by contamination of the many optical surfaces from the telescope primary mirror to the coronagraph mask. Particulate contamination that may accumulate even in clean room conditions over the period of integration, testing, and launch can cause performance degradation due to both coherent and incoherent scatter. While the coherent components can be compensated in broad-band light using a sequential deformable mirror architecture, incoherent scatter would remain. We show the challenges and effects of particulate contamination based on measurements and estimates, and discuss the requirements throughout the coronagraph system while accounting for the wavefront control system.
© (2009) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kunjithapatham Balasubramanian, Stuart Shaklan, and Amir Give'on "Stellar coronagraph performance impact due to particulate contamination and scatter", Proc. SPIE 7440, Techniques and Instrumentation for Detection of Exoplanets IV, 74400T (25 August 2009); https://doi.org/10.1117/12.825182
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Cited by 4 scholarly publications.
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KEYWORDS
Particles

Bidirectional reflectance transmission function

Coronagraphy

Contamination

Mirrors

Gold

Atmospheric particles

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