Open Access Paper
7 July 2006 The effects of instrumental elliptical polarization on stellar point spread function fine structure
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Abstract
We present a status report on a study on the effects of instrumental polarization on the fine structure of the stellar point spread function (PSF). These effects are important to understand because the the aberration caused by instrumental polarization on an otherwise diffraction-limited PSF will likely have have severe consequences for extreme high contrast imaging systems such as NASA's proposed Terrestrial Planet Finder (TPF) mission and the proposed NASA Eclipse mission. The report here, describing our efforts to examine these effects, includes two parts: 1) a numerical analysis of the effect of metallic reflection, with some polarization-specific retardation, on a spherical wavefront; 2) an experimental approach for observing this effect, along with a status report on preliminary laboratory results. The numerical analysis indicates that the inclusion of polarization-specific phase effects (retardation) results in a point spread function (PSF) aberration more severe than the amplitude (reflectivity) effects previously recorded in the literature. Preliminary in-lab results are consistent with our numerical predictions.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Joseph C. Carson, Brian D. Kern, John T. Trauger, and James B. Breckinridge "The effects of instrumental elliptical polarization on stellar point spread function fine structure", Proc. SPIE 6265, Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter, 62653M (7 July 2006); https://doi.org/10.1117/12.672518
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Point spread functions

Mirrors

Polarization

Reflectivity

Coating

Reflection

Space telescopes

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