A new method for calculating astronomical refraction in an atmosphere inhomogeneous in three dimensions

Details A new method for calculating astronomical refraction in an atmosphere inhomogeneous in three dimensions A new method for calculating astronomical refraction in an atmosphere inhomogeneous in three dimensions

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..695s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Nov.-Dec. 1983, p. 695-698) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Nov.-

Physics

Optics

Astronomical Photometry, Atmospheric Optics, Atmospheric Refraction, Inhomogeneity, Atmospheric Boundary Layer, Atmospheric Models, Atmospheric Stratification, Zenith

Scientific paper

Expressions for the astronomical refraction angles are obtained for a
three-dimensionally inhomogeneous model atmosphere. Typical experimental
data at large zenith distances are satisfactorily represented by
theoretical curves.

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