Fringe Position Measurement Based on Spatial Optical Path Difference Modulation

SUN Chang-Sheng; ZHU Yong-Tian; HU Zhong-Wen; XU Teng; MEI Rong

doi:10.3788/gzxb20164509.0912005

[1] WANG Hai-tao, CAI Jia-hui, WEI Peng, et al. Imaging analysis of optical synthetic aperture system with the immediate/para-immediate u-v coverage［J］. Acta Photonica Sinica, 2010, 39(2): 260-265.

[2] SHAO M, COLAVITA M M, HINES B E, et al. The Mark III stellar interferometer［J］. Astronomy and Astrophysics, 1988, 193: 357-371.

[3] ROBERTSON J G, IRELAND M J, TANGO W J, et al. Science and technology progress at the Sydney University Stellar Interferometer［C］. SPIE Astronomical Telescopes+ Instrumentation. International Society for Optics and Photonics, 2012: 84450N.

[4] COLAVITA M M,WIZINOWICH P L, AKESON R L, et al. The Keck interferometer［J］. Astronomical Society of the Pacific, 2013, 125(932): 1226.

[5] GLINDEMANN A, ABUTER R, CARBOGNANI F, et al. The VLT interferometer: A unique instrument for high-resolution astronomy［C］. Astronomical Telescopes and Instrumentation. International Society for Optics and Photonics, 2000: 2-12.

[6] CORCIONE L, BONINO D, BUSHER D F, et al. Fringe tracker for the VLTI spectro-imager［C］. SPIE Astronomical Telescopes+ Instrumentation. International Society for Optics and Photonics, 2008: 701345.

[7] GLINDEMANN A. Instrumental techniques［M］. Principles of Stellar Interferometry. Springer Berlin Heidelberg, 2011: 217-274.

[8] MOREL S, TRAUB W A, BREGMAN J D, et al. Fringe-tracking experiments at the IOTA interferometer［C］. Astronomical Telescopes and Instrumentation. International Society for Optics and Photonics, 2000: 506-513.

[9] GAI M, CORCIONE L, DELATGE L, et al. The FINITO fringe sensor for VLTI［C］.European Southern Observatory Conference and Workshop Proceedings. 2002, 58: 329.

[10] KERVELLA P, SéGRANSAN D, du FORESTO V C. Data reduction methods for single-mode optical interferometry-application to the VLTI two-telescopes beam combiner VINCI［J］. Astronomy & Astrophysics, 2004, 425(3): 1161-1174.

[11] LEVEQUE S A, WILHELM R, SALVADé Y, et al. Toward nanometer accuracy laser metrology for phase-referenced interferometry with the VLTI［C］. Astronomical Telescopes and Instrumentation. International Society for Optics and Photonics, 2003: 983-994.

[12] LAWSON P R. Phase and group delay estimation［C］.Principles of Long Baseline Stellar Interferometry. 2000: 113.

[13] GAI M, MENARDI S, CESARE S, et al. The vlti fringe sensors: FINITO and prima FSU［C］.SPIE Astronomical Telescopes+ Instrumentation. International Society for Optics and Photonics, 2004: 528-539.

[14] BLIND N, ABSIL O, LE BOUQUIN J B, et al. Optimized fringe sensors for the VLTI next generation instruments［J］. Astronomy & Astrophysics, 2011, 530: A121.

[15] LU Yi, FAN Wei-jun, KONG Ming. Measuring the tip-tilt angles of the active mirror in the stellar interferometer［J］. Acta Photonica Sinica, 2010, 39(6): 1111-1115.