Precise Astronomical Orientation Using Multiple Stars at Their Culmination and Analysis of Different Regression Models
Publication: Journal of Surveying Engineering
Volume 146, Issue 3
Abstract
Precise determination of the astronomical azimuth using the local hour angle (LHA) of Polaris is only applicable in northern middle latitudes. Therefore, to achieve fast and precise astronomical orientation in any part of the world, this study proposes continuous observations from the same station of multiple north stars and south stars at their culminating positions, thereby reducing the impact of errors in observation station longitude and time measurement. This method, which uses the regression model, determines the astronomical azimuth from the observation station to the ground target. Model validity is affected by various factors including sample size, data distribution, and data quality; therefore, suitable model conditions and individual characteristics of parametric and nonparametric regression are analyzed. Then, a two-step regression method comprising data binning followed by linear regression is proposed. Experimental data are subjected to direct linear regression, the summation of north and south star data followed by linear regression, nonparametric regression of summed data, and two-step regression of summed data. The two-step regression method produces the most accurate results that agree with those of the LHA method within a range of ±1.2120 × 10−6 rad (0.25″). Compared to the LHA method, the proposed method extends the geographical application range and eliminates the need for precise astronomical positioning prior to determining the orientation.
Get full access to this article
View all available purchase options and get full access to this article.
Data Availability Statement
Some or all data, models, or code generated or used during the study are available from the corresponding author by request (Figs. 2–12).
Acknowledgments
This research is funded by the National Nature Science Foundation of China (Nos. 41604011, 11673076, and 41704006), and the Independent Scientific Research Fund of Information Engineering University. The authors would like to thank Editage (www.editage.cn) for English language editing, the two reviewers for their comments on the manuscript, and the editor for the handling of the review process.
References
Balodimos, D. D., R. Korakitis, E. Lambrou, and G. Pantazis. 2003. “Fast and accurate determination of astronomical coordinates , , and azimuth, using a total station and GPS receiver.” Empire Surv. Rev. 37 (290): 269–275. https://doi.org/10.1179/sre.2003.37.290.269.
Carter, W. E., J. E. Pettey, and W. E. Strange. 1978. “The accuracy of astronomic azimuth determinations.” Bull. Géodésique 52 (2): 107–113. https://doi.org/10.1007/BF02521693.
Chauvenet, W. 1960. A manual of spherical and practical astronomy. Philadelphia: J.B. Lippincott.
Fox, J., and S. Weisberg. 2019. An R companion to applied regression. 3rd ed. Thousand Oaks, CA: SAGE Publications.
Gaivoronskii, S. V., S. B. Berkovich, N. I. Kotov, A. Y. Makhaev, R. N. Sadekov, and V. V. Tsodokova. 2015. “An automatic system for determining astronomical azimuth.” Meas. Tech. 58 (3): 280–285. https://doi.org/10.1007/s11018-015-0700-8.
Günter, D. R. 2009. Handbook of practical astronomy. New York: Springer.
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.
Hidalgo, S. J. T., M. C. Wu, S. M. Engel, and M. R. Kosorok. 2018. “Goodness-of-fit test for nonparametric regression models: Smoothing spline ANOVA models as example.” Comput. Stat. Data Anal. 122 (Jun): 135–155. https://doi.org/10.1016/j.csda.2018.01.004.
Lambrou, E., and G. Pantazis. 2013. “Astronomical azimuth determination by the hour angle of Polaris using ordinary total stations.” Empire Surv. Rev. 40 (308): 164–172. https://doi.org/10.1179/003962608X290951.
Li, C., J. Pu, Y. Zhan, Y. Zheng, C. Zhang, R. Wang, Y. Luo, and D. Wang. 2018. “Unified astronomical positioning and orientation model based on robust estimation.” J. Surv. Eng. 144 (2): 04017023. https://doi.org/10.1061/(ASCE)SU.1943-5428.0000248.
Li, G., J. Zhang, and S. Feng. 2016. Modern measurement error model. Beijing: Science Press.
Pu, J. Y., C. H. Li, Y. Zheng, and Y. H. Zhan. 2018. “Astronomical vessel heading determination based on simultaneously imaging the moon and the horizon.” J. Navig. 71 (5): 1247–1262. https://doi.org/10.1017/S0373463318000073.
Sheather, S. J., and M. C. Jones. 1991. “A reliable data-based bandwidth selection method for kernel density estimation.” J. R. Stat. Soc. Ser. B Methodol. 53 (3): 683–690. https://doi.org/10.1111/j.2517-6161.1991.tb01857.x.
Vasiljev, V., and O. Odalović. 1996. “Determination of astronomic azimuth using electronic theodolite.” Publications De L’Observatoire Astronomique De Beograd 54: 137–142.
Xia, J. B., C. Song, and J. Wu. 2007. Examination and application of Wild T4 theodolite. Wuhan, China: Wuhan University Press.
Xue, L. G. 2015. Modern nonparametric statistics. Beijing: Science Press.
Zhan, Y., Y. Zheng, and C. Zhang. 2016. “Astronomical azimuth determination by lunar observations.” J. Surv. Eng. 142 (2): 04015009. https://doi.org/10.1061/(ASCE)SU.1943-5428.0000158.
Zhan, Y., Y. Zheng, C. Zhang, Z. Li, and Z. Zhang. 2015. “Bright-star recognition algorithm and its application in astronomical azimuth determination.” Acta Geodaetica et Cartographica Sinica 44 (3): 257–263. https://doi.org/10.11947/j.AGCS.2015.20130557.
Information & Authors
Information
Published In
Copyright
©2020 American Society of Civil Engineers.
History
Received: Sep 28, 2019
Accepted: Feb 12, 2020
Published online: May 21, 2020
Published in print: Aug 1, 2020
Discussion open until: Oct 21, 2020
Authors
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.