• Optics and Precision Engineering
  • Vol. 27, Issue 11, 2321 (2019)
ZHANG Zhen-jun1,2,*, WANG Jian-cheng1,2,3, CHENG Xiang-ming1,2,3, ZHANG Yi-gong1,2,3, and MAO Wei1,3
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • 3[in Chinese]
  • show less
    DOI: 10.3788/ope.20192711.2321 Cite this Article
    ZHANG Zhen-jun, WANG Jian-cheng, CHENG Xiang-ming, ZHANG Yi-gong, MAO Wei. Measurement and calibration of optical axis changes for multi-function astronomical theodolite[J]. Optics and Precision Engineering, 2019, 27(11): 2321 Copy Citation Text show less
    References

    [1] MAO W, LI ZH M, FAN Y, et al.. Meridian Astronomy [M]. Beijing: Science Press, 1987. (in Chinese)

    [2] ZHAO M. Introduction to Astrometry [M]. Beijing: Science Press, 2012. (in Chinese)

    [3] WANG H, ZHAO Y X. Pointing model for LAMOST experiment set[J]. SPIE,2006,6267: 62673A.

    [4] MEEKS R L. Sources of uncertainty in telescope pointing models[J].SPIE,2004,5497: 140-148.

    [5] KIMBRELL J E. Deterministic errors in pointing and tracking systems I: identification and correction of static errors[J]. Proceedings of SPIE - The International Society for Optical Engineering, 1991, 1482: 415-424.

    [6] WALLACE P T . A rigorous algorithm for telescope pointing[J]. Proceedings of SPIE-The International Society for Optical Engineering, 2002: 125-136.

    [7] LI M M, LI ZH W, LIU CH ZH. Modeling and correction of static pointing error of level mounting telescope[J]. Laser & Infrared, 2017, 47(5): 624-629.(in Chinese)

    [8] LI ZH W, YANG W B, ZHANG N. Static pointing error of level mounting optoelectronic telescope[J]. Chinese Optics, 2015, 8(2): 263-269.(in Chinese)

    [9] LIU G Q, XIAO Q G, DENG L H, et al.. Detection and calibration of optical axes change for one meter solar telescope[J]. Chinese Journal of Lasers, 2013, 40(1): 206-211.(in Chinese)

    [10] ZHOU CH, YANG H B, WU X X, et al.. Structural analysis of ground-based large telescopes[J]. Opt. Precision Eng., 2011, 19(1): 138-145.(in Chinese)

    [11] WANG Y, HUANG Y, LI ZH F, et al.. Calibration of optical axis parallelism by using star for astronomical observation system[J]. Infrared and Laser Engineering, 2017, 46(5): 116-121.(in Chinese)

    [12] ZHANG CH, ZHOU B, SHEN X J, et al.. Study of the calculation method for accurately adjusting laser-range-finder′s three-optic-axes to parallel to each other[J]. Opt. Precision Eng., 2002, 10(6): 650-654.(in Chinese)

    [13] XIAO W J, MA D X, CHEN ZH B, et al.. Pointing uncertainty evaluation of optical axis in large-scale spatial angle measuring system[J]. Infrared and Laser Engineering, 2016, 45(11): 230-236.(in Chinese)

    [14] CHE X, JIA P, TIAN D P. A survey of line of sight control technology for airborne photoelectric payload[J]. Opt. Precision Eng., 2018,26(7): 1642-1652.(in Chinese)

    [15] YANG L B, LI Y H, WANG J, et al.. Alignment of Φ1000 mm primary mirror for photoelectric tracking system[J]. Opt. Precision Eng., 2018,26(7): 1633-1641. (in Chinese)

    [16] HU SH W, SONG X L, ZHANG H. Integrated system of azimuth structure for extremely large telescopes[J]. Opt. Precision Eng., 2018,26(4): 850-856.(in Chinese)

    [17] LI H F, DAI ZH X, XIANG J. Shaft parameters calibration of a ship-borne radar[J]. Telecommunication Engineering, 2018, 58(2): 157-161.(in Chinese)

    [18] MAO W , LI B H , YANG L , et al.. Constructing an observational model of the neutral atmospheric refraction delay from measured values of the astronomical refraction[J]. The Astronomical Journal, 2007, 134(5): 2054-2060.

    [19] MAO W, ZHANG H W, LI B H, et al.. A possible means of improving the accuracy of refraction delay correction of neutral atmosphere[J]. Chinese Astronomy and Astrophysics, 2007, 31(2): 211-220.

    [20] WANG J C, CHEN L F, YANG L, et al.. The principle of measuring unusual change of underground mass by optical astrometric instrument[J]. Geodesy and Geodynamics, 2012, 3(4): 32-38.

    [21] MAO W, JI K F, LI B H, et al.. CCD Astrometry [M]. Kunming: Yunnan Science and Technology Press, 2003. (in Chinese)

    [22] YANG L, TIE Q X, CHEN L F. The pointing variation of the optical axis in the LLMC[J]. Publications of the Yunnan Observatoty, 2000(4): 24-28.(in Chinese)

    [23] ZHANG Y G, LI B H, YANG L, et al.. An image processing system for a multi-function astronomical theodolite[J]. Astronomical Research & Technology, 2014, 11(1): 65-71.(in Chinese)

    [24] SU J, ZHANG Y G, YANG L, et al.. A new method to establish actual atmospheric refraction measurement model[J]. Journal of Yunnan University: Natural Sciences Edition, 2018, 40(2): 287-294. (in Chinese)

    CLP Journals

    [1] Baogang CHEN, Haojie XIA, Jin ZHANG, Jianli WANG, Yuyan CAO. Research on factors influencing the pointing accuracy of large telescopes and the correction model[J]. Optics and Precision Engineering, 2024, 32(20): 3017

    [2] Baogang CHEN, Haojie XIA, Jin ZHANG, Jianli WANG, Yuyan CAO. Research on factors influencing the pointing accuracy of large telescopes and the correction model[J]. Optics and Precision Engineering, 2024, 32(20): 3017

    ZHANG Zhen-jun, WANG Jian-cheng, CHENG Xiang-ming, ZHANG Yi-gong, MAO Wei. Measurement and calibration of optical axis changes for multi-function astronomical theodolite[J]. Optics and Precision Engineering, 2019, 27(11): 2321
    Download Citation