Abstract

Astronomical positioning can determine the astronomical longitude and latitude of a station based on observations of celestial bodies. The accuracy of astronomical positioning depends on the observation instruments, surveying environment, and geometric distribution of stellar observations. For astronomical theodolite, existing theories support that the best positioning accuracy can only be obtained with uniformly distributed stars on an equal-altitude circle. In fact, inhomogeneous distribution can also obtain the best positioning accuracy. To illustrate this problem, a quantitative index to determine the optimum geometric distribution of stellar observations by introducing the mean resultant length of vectors in directional statistics is proposed, providing a theoretical basis for studying high-precision astronomical positioning and automated star selection algorithms. Multiple optimum distributions of observations with constant numbers of stars during simulation experiments using the equal-altitude method have been demonstrated. Regarding the approximate equal-altitude method, the inhomogeneous distribution of stars guided by the conclusion described in this paper was also optimum. It could achieve the same accuracy as the uniform distribution. These results can aid in overcoming the limitations of the existing uniform distribution theory for astronomical positioning and provide a theoretical basis for achieving high-precision and high-efficiency astronomical positioning by inhomogeneous distribution stellar observations, especially when only a small number of stars can be observed.

Get full access to this article

View all available purchase options and get full access to this article.

Data Availability Statement

All models or codes supporting the results of this research can be obtained from the corresponding author upon reasonable request.

Acknowledgments

The authors would like to thank the National Natural Science Foundation of China (No. 42074013), the Natural Science Foundation of Henan Province (No. 212300410421), and the Young Elite Scientists Sponsorship Program of the Henan Association for Science and Technology (No. 2022HYTP008) for their financial support.

References

Albayrak, M., D. Willi, and S. Guillaume. 2022. “Field comparison of the total station-based QDaedalus and the zenith telescope-based CODIAC astrogeodetic systems for measurements of the deflection of the vertical.” Surv. Rev. 1–13. https://doi.org/10.1080/00396265.2022.2054108.
Chen, Z., C. Li, Y. Zheng, B. Chen, and D. He. 2019. “The minimum analysis of geometric dilution of precision in celestial positioning.” Acta. Geod. Cartogr. Sin. 48 (7): 879. https://doi.org/10.11947/j.AGCS.2019.20180479.
Guillaume, S. 2015. “Determination of a precise gravity field for the CLIC feasibility studies.” Ph.D. thesis, Dept. of Civil, Environmental and Geomatic Engineering, Eidgenössische Technische Hochschule ETH Zurich.
Guillaume, S., B. Bürki, S. Griffet, and H. M. Durand. 2012. “QDaedalus: Augmentation of total stations by CCD sensor for automated contactless high-precision metrology.” In FIG Working Week, 1–15. Rome: International Federation of Surveyors.
Halicioglu, K., R. Deniz, and H. Ozener. 2012. “Digital zenith camera system for Astro-Geodetic applications in Turkey.” J. Geod. Geoinf. 1 (2): 115–120. https://doi.org/10.9733/jgg.131212.1.
Hanada, H., et al. 2012. “Development of a digital zenith telescope for advanced astrometry.” Sci. China Phys. Mech. Astron. 55 (4): 723–732. https://doi.org/10.1007/s11433-012-4673-1.
Hauk, M., C. Hirt, and C. Ackermann. 2017. “Experiences with the QDaedalus system for astrogeodetic determination of deflections of the vertical.” Surv. Rev. 49 (355): 294–301. https://doi.org/10.1080/00396265.2016.1171960.
Hirt, C., and J. Flury. 2008. “Astronomical-topographic levelling using high-precision astrogeodetic vertical deflections and digital terrain model data.” J. Geod. 82 (4–5): 231–248. https://doi.org/10.1007/s00190-007-0173-x.
Hirt, C., and G. Seeber. 2008. “Accuracy analysis of vertical deflection data observed with the Hannover Digital Zenith Camera System TZK2-D.” J. Geod. 82 (6): 347–356. https://doi.org/10.1007/s00190-007-0184-7.
Li, C., Y. Zheng, C. Zhang, Y.-L. Yuan, Y.-Y. Lian, and P.-Y. Zhou. 2014. “Astronomical vessel position determination utilizing the optical super wide angle lens camera.” J. Navig. 67 (4): 633–649. https://doi.org/10.1017/S0373463314000058.
Mardia, K. V., and P. E. Jupp. 2000. Directional statistics, Wiley series in probability and statistics. Chichester, UK: Wiley.
Ning, X., and L. Liu. 2014. “A two-mode INS/CNS navigation method for lunar rovers.” IEEE Trans. Instrum. Meas. 63 (9): 2170–2179. https://doi.org/10.1109/TIM.2014.2307972.
Shi, C., et al. 2020. “Automatic astronomical survey method based on video measurement robot.” J. Surv. Eng. 146 (2): 04020002. https://doi.org/10.1061/(ASCE)SU.1943-5428.0000300.
Tian, L., J. Guo, Y. Han, X. Lu, W. Liu, Z. Wang, B. Wang, Z. Yin, and H. Wang. 2014. “Digital zenith telescope prototype of China.” Chin. Sci. Bull. 59 (17): 1978–1983. https://doi.org/10.1007/s11434-014-0256-z.
Torge, W., and J. Müller. 2012. Geodesy. Berlin: De Gruyter.
Wang, Q., M. Diao, W. Gao, M. Zhu, and S. Xiao. 2015. “Integrated navigation method of a marine strapdown inertial navigation system using a star sensor.” Meas. Sci. Technol. 26 (11): 115101. https://doi.org/10.1088/0957-0233/26/11/115101.
Wei, X., C. Cui, G. Wang, and X. Wan. 2019. “Autonomous positioning utilizing star sensor and inclinometer.” Measurement 131 (Jan): 132–142. https://doi.org/10.1016/j.measurement.2018.08.061.
Xue, S., and Y. Yang. 2015. “Positioning configurations with the lowest GDOP and their classification.” J. Geod. 89 (1): 49–71. https://doi.org/10.1007/s00190-014-0760-6.
Yang, Y., C. Zhang, and J. Lu. 2017. “Local observability analysis of star sensor installation errors in a SINS/CNS integration system for near-earth flight vehicles.” Sensors 17 (12): 167. https://doi.org/10.3390/s17010167.
Zhan, Y., Y. Zheng, C. Li, R. Wang, Y. Zhu, and Z. Chen. 2020. “High-accuracy absolute positioning for the stationary planetary rover by integrating the star sensor and inclinometer.” J. Field Rob. 37 (6): 1063–1076. https://doi.org/10.1002/rob.21944.

Information & Authors

Information

Published In

Go to Journal of Surveying Engineering
Journal of Surveying Engineering
Volume 149Issue 1February 2023

History

Received: Apr 8, 2022
Accepted: Jul 19, 2022
Published online: Nov 10, 2022
Published in print: Feb 1, 2023
Discussion open until: Apr 10, 2023

Permissions

Request permissions for this article.

Authors

Affiliations

Postgraduate, Geospatial Information College, Information Engineering Univ., Zhengzhou 450001, China. ORCID: https://orcid.org/0000-0002-2593-6310. Email: [email protected]
Chonghui Li [email protected]
Lecturer, Geospatial Information College, Information Engineering Univ., Zhengzhou 450001, China; Postdoctoral, Dept. of Geodesy, State Key Laboratory of Geo-information Engineering, Xi’an 710054 China. Email: [email protected]
Professor, Geospatial Information College, Information Engineering Univ., Zhengzhou 450001, China (corresponding author). Email: [email protected]
Lecturer, Geospatial Information College, Information Engineering Univ., Zhengzhou 450001, China. Email: [email protected]
Doctoral Student, Geospatial Information College, Information Engineering Univ., Zhengzhou 450001, China. ORCID: https://orcid.org/0000-0003-1710-3973. Email: [email protected]
Postgraduate, Geospatial Information College, Information Engineering Univ., Zhengzhou 450001, China. Email: [email protected]
Postgraduate, Geospatial Information College, Information Engineering Univ., Zhengzhou 450001, China. Email: [email protected]
Postgraduate, Geospatial Information College, Information Engineering Univ., Zhengzhou 450001, China. Email: [email protected]

Metrics & Citations

Metrics

Citations

Download citation

If you have the appropriate software installed, you can download article citation data to the citation manager of your choice. Simply select your manager software from the list below and click Download.

View Options

Get Access

Access content

Please select your options to get access

Log in/Register Log in via your institution (Shibboleth)
ASCE Members: Please log in to see member pricing

Purchase

Save for later Information on ASCE Library Cards
ASCE Library Cards let you download journal articles, proceedings papers, and available book chapters across the entire ASCE Library platform. ASCE Library Cards remain active for 24 months or until all downloads are used. Note: This content will be debited as one download at time of checkout.

Terms of Use: ASCE Library Cards are for individual, personal use only. Reselling, republishing, or forwarding the materials to libraries or reading rooms is prohibited.
ASCE Library Card (5 downloads)
$105.00
Add to cart
ASCE Library Card (20 downloads)
$280.00
Add to cart
Buy Single Article
$35.00
Add to cart

Get Access

Access content

Please select your options to get access

Log in/Register Log in via your institution (Shibboleth)
ASCE Members: Please log in to see member pricing

Purchase

Save for later Information on ASCE Library Cards
ASCE Library Cards let you download journal articles, proceedings papers, and available book chapters across the entire ASCE Library platform. ASCE Library Cards remain active for 24 months or until all downloads are used. Note: This content will be debited as one download at time of checkout.

Terms of Use: ASCE Library Cards are for individual, personal use only. Reselling, republishing, or forwarding the materials to libraries or reading rooms is prohibited.
ASCE Library Card (5 downloads)
$105.00
Add to cart
ASCE Library Card (20 downloads)
$280.00
Add to cart
Buy Single Article
$35.00
Add to cart

Media

Figures

Other

Tables

Share

Share

Copy the content Link

Share with email

Email a colleague

Share