Astroclimate parameters of the Kyiv observatories

dc.contributor.author	Rieznik, K.
dc.contributor.author	Reshetnyk, V.M.
dc.date.accessioned	2017-06-06T18:35:46Z
dc.date.available	2017-06-06T18:35:46Z
dc.date.issued	2012
dc.description.abstract	Astroclimate parameters such as the atmospheric extinction, the night-sky brightness, and the seeing are studied using the observational data obtained at some Kyiv observatories. The first parameter is determined using the brief Bouguer method. The night-sky brightness is calculated using the images of standard stars in different filters. And the seeing is estimated basing on the FWHM of star profiles obtained during a set of observations at Kyiv observatories.	uk_UA
dc.description.sponsorship	We would like to thank Simon A. O. for the granted observational data.	uk_UA
dc.identifier.citation	Astroclimate parameters of the Kyiv observatories / K. Rieznik, V.M. Reshetnyk // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 203-205. — Бібліогр.: 3 назв. — англ.	uk_UA
dc.identifier.issn	2227-1481
dc.identifier.uri	https://nasplib.isofts.kiev.ua/handle/123456789/119407
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.status	published earlier	uk_UA
dc.title	Astroclimate parameters of the Kyiv observatories	uk_UA
dc.type	Article	uk_UA

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