Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS

The investigations of the atmospheric turbulence instability are carried out. The observations of different stars and different positions of stars in the sky performed with the AZT-2 telescope (diameter of 0.7 m) of the Main Astronomical Observatory, Kyiv, Ukraine, and at the Optical Ground Station...

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Опубліковано в: :Кинематика и физика небесных тел
Дата:2005
Автори: Kuz'kov, V., Andruk, V., Sizonenko, Yu., Sodnik, Z.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2005
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Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/79722
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS / V. Kuz'kov, V. Andruk, Yu. Sizonenko, Z. Sodnik // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 561-564. — Бібліогр.: 5 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-79722
record_format dspace
spelling Kuz'kov, V.
Andruk, V.
Sizonenko, Yu.
Sodnik, Z.
2015-04-03T20:32:20Z
2015-04-03T20:32:20Z
2005
Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS / V. Kuz'kov, V. Andruk, Yu. Sizonenko, Z. Sodnik // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 561-564. — Бібліогр.: 5 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79722
The investigations of the atmospheric turbulence instability are carried out. The observations of different stars and different positions of stars in the sky performed with the AZT-2 telescope (diameter of 0.7 m) of the Main Astronomical Observatory, Kyiv, Ukraine, and at the Optical Ground Station (the 1.0-m telescope) of ESA at Canary Islands are described. Short exposures (40 ms) with CCD cameras in focal plane of objectives with the filters were used. The calculations of middle positions of star images were performed. The deviation of star’s image positions from the middle position was also performed. The atmospheric attenuation and FWHM (Full Width Half Maximum) function were calculated using the MIDAS/ROMAFOT software package. The results of analyses of experimental data obtained due to observations in different regions are also presented.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
spellingShingle Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
Kuz'kov, V.
Andruk, V.
Sizonenko, Yu.
Sodnik, Z.
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
title_short Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
title_full Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
title_fullStr Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
title_full_unstemmed Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
title_sort investigation of atmospheric instability for communication experiments with the esa's geostationary satellite artemis
author Kuz'kov, V.
Andruk, V.
Sizonenko, Yu.
Sodnik, Z.
author_facet Kuz'kov, V.
Andruk, V.
Sizonenko, Yu.
Sodnik, Z.
topic MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
topic_facet MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
publishDate 2005
language English
container_title Кинематика и физика небесных тел
publisher Головна астрономічна обсерваторія НАН України
format Article
description The investigations of the atmospheric turbulence instability are carried out. The observations of different stars and different positions of stars in the sky performed with the AZT-2 telescope (diameter of 0.7 m) of the Main Astronomical Observatory, Kyiv, Ukraine, and at the Optical Ground Station (the 1.0-m telescope) of ESA at Canary Islands are described. Short exposures (40 ms) with CCD cameras in focal plane of objectives with the filters were used. The calculations of middle positions of star images were performed. The deviation of star’s image positions from the middle position was also performed. The atmospheric attenuation and FWHM (Full Width Half Maximum) function were calculated using the MIDAS/ROMAFOT software package. The results of analyses of experimental data obtained due to observations in different regions are also presented.
issn 0233-7665
url https://nasplib.isofts.kiev.ua/handle/123456789/79722
citation_txt Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS / V. Kuz'kov, V. Andruk, Yu. Sizonenko, Z. Sodnik // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 561-564. — Бібліогр.: 5 назв. — англ.
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AT sizonenkoyu investigationofatmosphericinstabilityforcommunicationexperimentswiththeesasgeostationarysatelliteartemis
AT sodnikz investigationofatmosphericinstabilityforcommunicationexperimentswiththeesasgeostationarysatelliteartemis
first_indexed 2025-11-30T15:56:17Z
last_indexed 2025-11-30T15:56:17Z
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