International Conference on Space Optics — ICSO 2006 2017
DOI: 10.1117/12.2308157
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The HSOB GAIA: a cryogenic high stability cesic optical bench for missions requiring sub-nanometric optical stability

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(5 citation statements)
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“…The very good performance of SAGEIS-CSO laser metrologic system has allowed the HSOB tests to be brought to a successful conclusion [1]. This test campaign has also formed a good basis to understand the technical limitations of this system when dedicated to the measurements of sub-nanometric displacements.…”
Section: Resultsmentioning
confidence: 94%
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“…The very good performance of SAGEIS-CSO laser metrologic system has allowed the HSOB tests to be brought to a successful conclusion [1]. This test campaign has also formed a good basis to understand the technical limitations of this system when dedicated to the measurements of sub-nanometric displacements.…”
Section: Resultsmentioning
confidence: 94%
“…measuring arm output (2) measuring arm input (3) injection point (1) interferometric area single-mode waveguide output single-mode waveguides (6) curved reference guide reference photometric arm (5) measuring photometric arm (4) : junction measuring arm output (2) measuring arm input (3) injection point (1) interferometric area single-mode waveguide output single-mode waveguides (6) curved reference guide reference photometric arm (5) measuring photometric arm (4) : junction a straight input waveguide, in which we inject the optical beam coming from a single-mode fibre; a splitting junction, dividing this beam into two arms: the measuring one (straight) and the reference one (curved). This junction can be an asymmetric Y-junction or a directional coupler; a return straight waveguide, in which we collect the measuring beam coming back from the corner cube; a loop, allowing to drive the reference beam into an area where it interferes with the measuring beam.…”
Section: General Principlementioning
confidence: 99%
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“…This material combination was proved to offer the needed dimensional stability at the nanometer level at room temperature. [7] The Global Astrometric Interferometer for Astrophysics [8] (GAIA) mission is another example where dimensional stability is critical: its mirrors and support are made of silicon carbide structures and need stabilities at the picometer and picoradian level in a cold environment [9,10] (%100 K). The future spaceborne gravitational wave detector, LISA, will also require extremely stable optical assemblies such as optical benches and telescopes.…”
Section: Introductionmentioning
confidence: 99%