Detailed Information on Publication Record
2002
Atmospheric Extinction Derived from Cometary Observations
SVOREŇ, Ján, Jozef ŽIŽŇOVSKÝ, Zdeněk MIKULÁŠEK and Jozef TREMKOBasic information
Original name
Atmospheric Extinction Derived from Cometary Observations
Authors
SVOREŇ, Ján (703 Slovakia), Jozef ŽIŽŇOVSKÝ (703 Slovakia), Zdeněk MIKULÁŠEK (203 Czech Republic, guarantor) and Jozef TREMKO (703 Slovakia)
Edition
NATO Science Series. Dordrecht/Boston/London, Optics of Cosmic Dust, proceedings of a NATO Adv. Research Workshop Slovak Republic. p. 183-202, 2002
Publisher
Kluwer Academic Publishers,
Other information
Language
English
Type of outcome
Stať ve sborníku
Field of Study
10308 Astronomy
Country of publisher
Netherlands
Confidentiality degree
není předmětem státního či obchodního tajemství
RIV identification code
RIV/00216224:14310/02:00006300
Organization unit
Faculty of Science
ISBN
1-4020-0819-8
UT WoS
000179729200012
Keywords in English
atmospheric extinction; IHW photometric system; dust; comets
Tags
International impact
Změněno: 24/6/2009 22:36, prof. RNDr. Zdeněk Mikulášek, CSc.
V originále
Extinction measurements in the intermediate band IHW/IAU system obtained during the observations of bright comets 1P/Halley in 1985/86, 23P/Brorsen-Metcalf in 1989 and C/Austin in 1990 are used in this study. 78 measurements in 21 observational nights cover all the parts of year with the exception of spring with cloudy weather in our mountain site and June with the shortest observational nights. Average extinction coefficients are derived in the paper and some conclusions of common validity (in central European conditions) are formulated. The results of IHW/IAU extinction study have been compared with the results of UBV extinction coefficients gained mostly as a by-product of the photoelectric photometry of variable stars (407 nights in the period from 1962 to 1995). Seasonal variations of atmospheric extinction are discussed.
In Czech
Extinction measurements in the intermediate band IHW/IAU system obtained during the observations of bright comets 1P/Halley in 1985/86, 23P/Brorsen-Metcalf in 1989 and C/Austin in 1990 are used in this study. 78 measurements in 21 observational nights cover all the parts of year with the exception of spring with cloudy weather in our mountain site and June with the shortest observational nights. Average extinction coefficients are derived in the paper and some conclusions of common validity (in central European conditions) are formulated. The results of IHW/IAU extinction study have been compared with the results of UBV extinction coefficients gained mostly as a by-product of the photoelectric photometry of variable stars (407 nights in the period from 1962 to 1995). Seasonal variations of atmospheric extinction are discussed.
Links
| GA205/02/0445, research and development project |
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| ME 131, research and development project |
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