Paper
21 September 2012 The thermal sieve: a diffractive baffle that provides thermal isolation of a cryogenic optical system from an ambient temperature collimator
James H. Burge, Dae Wook Kim
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Abstract
We present the thermal sieve, which is a diffractive baffle that provides thermal isolation between an ambient collimator and a cryogenic optical system being measured. The baffle uses several parallel plates with holes in them. The holes are lined up to allow the collimated light to pass, but the view factor for thermal radiation is greatly reduced. A particular design is shown here that allows less than 0.25 W/m2 thermal transfer and degrades the test wavefront by only 3 nm rms.
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James H. Burge and Dae Wook Kim "The thermal sieve: a diffractive baffle that provides thermal isolation of a cryogenic optical system from an ambient temperature collimator", Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84421L (21 September 2012); https://doi.org/10.1117/12.927789
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KEYWORDS
Collimators

Optical testing

Cryogenics

Wavefronts

Collimation

Diffraction

Optical cryogenics

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