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    Publication Date: 2019-07-13
    Description: Delay lines provide the path-length compensation that makes the measurement of interference fringes possible. When used for nulling interferometry, the delay line must control path-lengths so that the null is stable and controlled throughout the measurement. We report on a low noise, low disturbance, and high bandwidth optical delay line capable of meeting the TPF interferometer optical path length control requirements at cryogenic temperatures.
    Keywords: Astronomy
    Type: Proceedings of SPIE Astronomical Telescopes and Instrumentation, Scottish Exhibition Center|SPIE Astronomical Telescopes and Instrumentation, Scottish Exhibition Center; Jun 21, 2004 - Jun 25, 2004; Glasgow, Scotland; United Kingdom
    Format: text
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