Paper
10 July 2018 Simulation analysis of the photographic noncoincidence between fiber ends and light spots under integrating sphere light source
Author Affiliations +
Abstract
Fiber spectroscopic telescopes, such as LAMOST, require accurate alignment between the fiber ends and their corresponding celestial targets. In the measurement, the center of a light spot obtained through gray centroid method is regarded as the center of a fiber end. Nevertheless, we’ve observed that these two centers don’t coincide under wide visual angles when integrating sphere (Built in light source for bromine tungsten lamp) is used as light source. Basing on these phenomena we observed, this paper proposes a hypothesis that the maximum intensity of the light transmitted by the optical fiber to the end of the optical fiber is outside the end of the fiber. The intensity distribution at the output end of fibers under integrating sphere light source is simulated in this study. Keywords: accurate alignment
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Juan Luo, Yonggang Gu, Ye Zhu, and Chao Zhai "Simulation analysis of the photographic noncoincidence between fiber ends and light spots under integrating sphere light source", Proc. SPIE 10706, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation III, 107064B (10 July 2018); https://doi.org/10.1117/12.2311818
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Light sources

Optical fibers

Light

Integrating spheres

Lamps

Bromine

Tungsten

RELATED CONTENT

Sensitivity of an illumination system to lamp flicker
Proceedings of SPIE (September 23 2008)
Computing illumination-bundle focusing by lens systems
Proceedings of SPIE (January 01 1991)
Study on chroma balance based on grating spectrometer for LED
Proceedings of SPIE (November 20 2007)
S+C+L ultra broadband light source research
Proceedings of SPIE (October 15 2012)

Back to Top