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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Видавець:Головна астрономічна обсерваторія НАН України
Дата:2005
Автори: Kuz'kov, V., Andruk V., Andruk V., Sizonenko, Yu., Sodnik, Z.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2005
Назва видання:Кинематика и физика небесных тел
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Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/79722
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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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id irk-123456789-79722
record_format dspace
spelling irk-123456789-797222015-04-04T03:02:36Z Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS Kuz'kov, V. Andruk V., Andruk V. Sizonenko, Yu. Sodnik, Z. MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics 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. 2005 Article 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 http://dspace.nbuv.gov.ua/handle/123456789/79722 en Кинематика и физика небесных тел Головна астрономічна обсерваторія НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
spellingShingle MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
Kuz'kov, V.
Andruk V., Andruk V.
Sizonenko, Yu.
Sodnik, Z.
Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
Кинематика и физика небесных тел
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.
format Article
author Kuz'kov, V.
Andruk V., Andruk V.
Sizonenko, Yu.
Sodnik, Z.
author_facet Kuz'kov, V.
Andruk V., Andruk V.
Sizonenko, Yu.
Sodnik, Z.
author_sort Kuz'kov, V.
title Investigation of atmospheric instability for communication experiments with the ESA's geostationary satellite ARTEMIS
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
publisher Головна астрономічна обсерваторія НАН України
publishDate 2005
topic_facet MS6: New Trends, Research Directions, and Perspective Programs in the Field of Astronomy and Astrophysics
url http://dspace.nbuv.gov.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.
series Кинематика и физика небесных тел
work_keys_str_mv AT kuzkovv investigationofatmosphericinstabilityforcommunicationexperimentswiththeesasgeostationarysatelliteartemis
AT andrukvandrukv investigationofatmosphericinstabilityforcommunicationexperimentswiththeesasgeostationarysatelliteartemis
AT sizonenkoyu investigationofatmosphericinstabilityforcommunicationexperimentswiththeesasgeostationarysatelliteartemis
AT sodnikz investigationofatmosphericinstabilityforcommunicationexperimentswiththeesasgeostationarysatelliteartemis
first_indexed 2023-10-18T19:19:22Z
last_indexed 2023-10-18T19:19:22Z
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