2012
DOI: 10.1016/j.cryogenics.2011.10.004
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High-precision CTE measurement of hybrid C/SiC composite for cryogenic space telescopes

Abstract: This paper presents highly precise measurements of thermal expansion of a "hybrid" carbon-fiber reinforced silicon carbide composite, HB-Cesic®a trademark of ECM, in the temperature region of ~310 10K. Whilst C/SiC composites have been considered to be promising for the mirrors and other structures of space-borne cryogenic telescopes, the anisotropic thermal expansion has been a potential disadvantage of this material. HB-Cesic® is a newly developed composite using a mixture of different types of chopped, shor… Show more

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Cited by 21 publications
(9 citation statements)
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“…All absolute CTE measurements are made with use of interferometric heads giving quite good accuracy but several laboratories claim some difficulties [5], [6], [7], [8], [9], [10]. For its Zerodur® material, Schott claims improved dilatometric measurements with an accuracy of +/-0.0062 .…”
Section: A State Of the Art Through The Literaturementioning
confidence: 99%
“…All absolute CTE measurements are made with use of interferometric heads giving quite good accuracy but several laboratories claim some difficulties [5], [6], [7], [8], [9], [10]. For its Zerodur® material, Schott claims improved dilatometric measurements with an accuracy of +/-0.0062 .…”
Section: A State Of the Art Through The Literaturementioning
confidence: 99%
“…in semiconductor industry, precision optics or in aerospace applications 1,2 . To enable high accuracy operation many measurement systems use reference material samples as calibration standards.…”
Section: Introductionmentioning
confidence: 99%
“…Thermal expansion of ultra stable materials at cryogenic temperatures is of increasing scientific interest driven by technological applications [2][3][4][5][6][7] . High accuracy CTE values at cryogenic temperatures are essential e.g.…”
Section: Introductionmentioning
confidence: 99%
“…Though the tip-tilt mirror is a moving part, it is expected to enable more accurate EChO adopts a 1.5m class telescope with spectrometers, and covers the wavelength region of 0. [4][5][6][7][8][9][10][11][12][13][14][15][16] microns (e.g., Tinetti et al 2012). If SPICA will the wideband infrared spectrometer, it will be complementally with these dedicated missions because of difference of stability of the system (available stability/dedicated stability), telescope time (part time of multi-purpose mission/full time) , and the size of the telescope aperture.…”
Section: Applicationmentioning
confidence: 99%
“…Therefore, next generation space-borne infrared telescopes, for instance, the Space Infrared telescope for Cosmology and Astrophysics (SPICA; e.g., Nakagawa 2010 and its references) and the James Webb Space Telescope (JWST; e.g., Clampin 2008), will be important platforms for such observations because of their large aperture, wide infrared wavelength coverage, capability of observations free from air turbulence, and high stability of optics at cryogenic temperature (Enya et al 2007;2012). With taking these features into consideration, this paper presents a conceptual design for a wideband infrared spectrometer designed specifically for observing transiting exoplanets with space-borne infrared telescopes.…”
Section: Introductionmentioning
confidence: 99%