The theory of astronomical refraction in a three-dimensionally inhomogeneous atmosphere

Details The theory of astronomical refraction in a three-dimensionally inhomogeneous atmosphere The theory of astronomical refraction in a three-dimensionally inhomogeneous atmosphere

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991opat....4.1025p&link_type=abstract

Optika Atmosfery (ISSN 0235-277X), vol. 4, Oct. 1991, p. 1025-1029. In Russian.

Physics

Optics

Atmospheric Refraction, Electromagnetic Radiation, Refracted Waves, Seeing (Astronomy), Three Dimensional Models, Atmospheric Optics, Geometrical Optics, Inhomogeneity

Scientific paper

Formulas for calculating vertical and lateral astronomical refraction describing the refraction anomalies as functions of the azimuth, elevation angle, and atmospheric parameters above the observation point are derived within the framework of a model of a three-dimensionally inhomogeneous atmosphere. A theory which is correct for an arbitrary three-dimensionally inhomogeneous spatial distribution of the air refraction index is constructed.

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