Abstract
The results of detailed calculations on first order Rayleigh- and Mie-scattering in the Earth's atmosphere illuminated by the Milky Way and the Zodiacal Light are presented. The influence of various independent parameters, as optical depth of the Rayleigh- and Mie-component and position of Milky Way and Zodiacal Light, is discussed. Linear and circular polarization of the scattered light are considered. The results are compared with the procedures commonly applied in reducing photometric observations of extended sources of the night sky. It is shown that a substantial part of the discrepancies between the brightness distributions of Zodiacal Light resp. Milky Way given by different authors is due to an inaccurate treatment of the atmospheric scattered light.
Author information
Authors and Affiliations
Editor information
Rights and permissions
Copyright information
© 1976 Springer-Verlag
About this paper
Cite this paper
Staude, H.J. (1976). Scattering in the earth's atmosphere: Calculations for milky way and zodiacal light as extended sources. In: Elsässer, H., Fechting, H. (eds) Interplanetary Dust and Zodiacal Light. Lecture Notes in Physics, vol 48. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-07615-8_466
Download citation
DOI: https://doi.org/10.1007/3-540-07615-8_466
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-07615-5
Online ISBN: 978-3-540-38133-4
eBook Packages: Springer Book Archive