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.
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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 (203 Česká republika, garant), Jiří PAPOUŠEK (203 Česká republika), Jozef TREMKO (703 Slovensko) a Jozef ŽIŽŇOVSKÝ (703 Slovensko).
Vydání Contributions of the Astronomical Observatory Skalnaté Pleso, Tatranska Lomnica, Slovak Republic, Astronomický ústav SAV, 2001, 1335-1842.
Další údaje
Originální jazyk angličtina
Typ výsledku Článek v odborném periodiku
Obor 10308 Astronomy
Stát vydavatele Slovensko
Utajení není předmětem státního či obchodního tajemství
Kód RIV RIV/00216224:14310/01:00006019
Organizační jednotka Přírodovědecká fakulta
Klíčová slova anglicky extinction: atmospheric
Štítky extinction: atmospheric
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnil: prof. RNDr. Zdeněk Mikulášek, CSc., učo 534. Změněno: 21. 5. 2003 11:06.
Anotace
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.
Anotace 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.
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