What is it about?

Satellite navigation systems have a fundamental defect: a vulnerability to hacking and spoofing. Thus, the problem of searching for new sources of navigational information arises. One of such sources is the classic navigation on the stars, the Moon, the Sun, and the planets of the solar system. The accuracy of such navigation is determined by the accuracy of the local vertical direction measuring. Local vertical direction is often determined from the image of the horizon line. Accordingly, the stability of the horizon line has the most direct effect on the navigation precision.

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Why is it important?

The horizon image is formed by the complicated processes of light propagation, absorption, scattering and refraction in the atmosphere. The result of this process heavily depends on the altitude of observation, aerosol concentration, Sun position as well as pressure and temperature variations in atmosphere. The existing approximate models of horizon image forming sometimes demonstrate results that are far from reality. Thus, it is mainly experimental studies that are needed.

Perspectives

Writing this article we hope that the processes of image forming at long-range and very long-range distances will be studied more carefully by experimental methods.

PhD, Associate Professor Vladimir Aleksandrovich Grishin
Space Research Institute of the Russian Academy of Sciences

Read the Original

This page is a summary of: Horizon Line Stability Observations over the Sea, Journal of Navigation, October 2017, Cambridge University Press,
DOI: 10.1017/s0373463317000650.
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