Atmospheric extinction at the Brno and Skalnate Pleso Observatories II. Interpretaion of Observations. Models of Extinction. Long-term and Seasonal Variations. Prediction.

MIKULÁŠEK, Zdeněk; Jiří PAPOUŠEK; Jozef TREMKO a Jozef ŽIŽŇOVSKÝ. Atmospheric extinction at the Brno and Skalnate Pleso Observatories II. Interpretaion of Observations. Models of Extinction. Long-term and Seasonal Variations. Prediction. Contributions of the Astronomical Observatory Skalnaté Pleso. Tatranska Lomnica, Slovak Republic: Astronomický ústav SAV, 2001, roč. 31, č. 2, s. 90-118. ISSN 1335-1842.

Základní údaje

Originální název

Atmospheric extinction at the Brno and Skalnate Pleso Observatories II. Interpretaion of Observations. Models of Extinction. Long-term and Seasonal Variations. Prediction.

Autoři

MIKULÁŠEK, Zdeněk; Jiří PAPOUŠEK; Jozef TREMKO a Jozef ŽIŽŇOVSKÝ

Vydání

Contributions of the Astronomical Observatory Skalnaté Pleso, Tatranska Lomnica, Slovak Republic, Astronomický ústav SAV, 2001, 1335-1842

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Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Slovensko

Utajení

není předmětem státního či obchodního tajemství

Označené pro přenos do RIV

Ano

Kód RIV

RIV/00216224:14310/01:00006019

Organizační jednotka

Přírodovědecká fakulta

Klíčová slova anglicky

extinction: atmospheric

Štítky

extinction: atmospheric

Příznaky

Mezinárodní význam, Recenzováno

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Anotace

V originále

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.

Česky

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.