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Atmospheric extinction at the Brno and Skalnate Pleso Observatories II. Interpretaion of Observations. Models of Extinction. Long-term and Seasonal Variations. Prediction.
Authors | |
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Year of publication | 2001 |
Type | Article in Periodical |
Magazine / Source | Contributions of the Astronomical Observatory Skalnaté Pleso |
MU Faculty or unit | |
Citation | |
Field | Astronomy and astrophysics |
Keywords | extinction: atmospheric |
Description | The behaviour of atmosperic extinction at the Skalnate Pleso Observatory can be satisfactorily described by a standard two-component model consisting of more or less constant component given namely by the Rayleigh scattering and a variable one caused by a scattering of light on dust particles. In order to explain properties of Brno extincion we introduce an additional, variable "particular extinction" acting mainly in U and B colours. Long-term and seasonal variations of both variable components of extinction in the B colour have been thoroughly investigated. The proposed extinction models are confronted with observations in all colours of UBV system. Trends of the UBVRI extinctions are discussed. |