Astronomical refraction theory for a three-dimensional model atmosphere

Details Astronomical refraction theory for a three-dimensional model atmosphere Astronomical refraction theory for a three-dimensional model atmosphere

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56..672s&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, May-June 1979, p. 672-682. In Russian.

Mathematics

Logic

Astronomy, Atmospheric Models, Atmospheric Refraction, Meteorological Parameters, Three Dimensional Models, Angles (Geometry), Atmospheric Boundary Layer, Azimuth, Differential Equations, Perturbation Theory, Zenith

Scientific paper

Equations for calculating astronomical refraction angles from zenith distance and azimuth are obtained for an asymmetric three-dimensional model atmosphere. Solutions based on perturbation techniques and the Bernoulli method are examined. The main requirements for collection of the meteorological data necessary for the refraction-angle computations are outlined for the cases of the atmospheric ground layer, the boundary layer, and the free atmosphere to heights of 35 and 75 km.

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