Atmospheric distribution model

Details Atmospheric distribution model Atmospheric distribution model

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005pnaoc...2..278z&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 2, No.

Astronomy and Astrophysics

Astronomy

Atmospheric Distribution Model, Non-Spherical Symmetry, Astronomical Refraction, Refraction Delay

Scientific paper

Atmospheric vertical distributions and high altitude surveying techniques are described briefly. The reason why the atmospheric spherically symmetric distribution models are only adopted at present is analyzed. It is demonstrated that astronomical refraction measured models varied with change in observing stations and observation directions already have characteristics of non-spherically symmetric distribution of the real atmosphere over the observing stations so that there is no need to find or build atmospheric distribution models varied with change in topography and seasons. With the measured models, influences of ill selection of atmospheric distribution models can be avoided. All these from one side will ensure success in improving accuracies of the astronomical refraction correction and the radio wave refraction correction and the radio wave refraction delay correction.

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