1 January 2008 MONS space telescope, part 2: analysis of very high stray-light rejection
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Optical Engineering, 47(1), 013001 (2008). doi:10.1117/1.2831662
Abstract
We develop new visualization and diagnostics techniques for the analysis of the mechanical causes of second-order scattered light, applying these to the stray-light analysis of the MONS space telescope, whose scientific aim is the measurement of low-amplitude photometric oscillations in stars. The telescope is designed to detect amplitudes of 1 part per million, requiring a high stray-light rejection factor, and is thus an ideal subject for this work. The analysis involved determining stray-light cases and then using an innovative approach to efficient high-order ray tracing to produce detailed predictions of the stray-light flux distributions. In addition to demonstrating the utility of the approaches developed here, the results of the analysis show that the MONS space telescope design meets the stray-light rejection requirements.
Christopher R. Boshuizen, Tim R. Bedding, Murray Leigh Pfitzner, Mark G. Grimminck, Hans Kjeldsen, A. G. Monger, "MONS space telescope, part 2: analysis of very high stray-light rejection," Optical Engineering 47(1), 013001 (1 January 2008). http://dx.doi.org/10.1117/1.2831662
JOURNAL ARTICLE
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KEYWORDS
Scattering

Sensors

Space telescopes

Light scattering

Stray light

Telescopes

Mirrors

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