Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data

Some results of study for high-resolution spectra of Jupiter and Saturn atmospheres are presented. The spectral data are derived with the help of the coude echelle spectrometer installed on the 2-m telescope at the Terskol Observatory (the Northern Caucasus). The investigations are carried out with...

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Veröffentlicht in:Кинематика и физика небесных тел
Datum:2005
Hauptverfasser: Kuznyetsova, Yu.G., Vid'machenko, A.P.
Format: Artikel
Sprache:English
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2005
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Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/79703
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Zitieren:Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data / Yu.G. Kuznyetsova, A.P. Vid'machenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 480-482. — Бібліогр.: 5 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-79703
record_format dspace
spelling Kuznyetsova, Yu.G.
Vid'machenko, A.P.
2015-04-03T19:50:20Z
2015-04-03T19:50:20Z
2005
Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data / Yu.G. Kuznyetsova, A.P. Vid'machenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 480-482. — Бібліогр.: 5 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79703
Some results of study for high-resolution spectra of Jupiter and Saturn atmospheres are presented. The spectral data are derived with the help of the coude echelle spectrometer installed on the 2-m telescope at the Terskol Observatory (the Northern Caucasus). The investigations are carried out with consideration for Raman light scattering. Calculations for molecular scattering effect in the atmospheres of giant planets are made for visible part of the spectrum. Wavelengths of Fraunhofer lines and their strongest ghosts caused by the rotational S(0), S(1), O(2) and the vibrational Q₁(1) transitions are used.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS5: Dynamics and Physics of Solar System Bodies
Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data
spellingShingle Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data
Kuznyetsova, Yu.G.
Vid'machenko, A.P.
MS5: Dynamics and Physics of Solar System Bodies
title_short Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data
title_full Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data
title_fullStr Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data
title_full_unstemmed Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data
title_sort raman scattering effect in atmospheres of giant planets of the solar system from high-resolution spectral data
author Kuznyetsova, Yu.G.
Vid'machenko, A.P.
author_facet Kuznyetsova, Yu.G.
Vid'machenko, A.P.
topic MS5: Dynamics and Physics of Solar System Bodies
topic_facet MS5: Dynamics and Physics of Solar System Bodies
publishDate 2005
language English
container_title Кинематика и физика небесных тел
publisher Головна астрономічна обсерваторія НАН України
format Article
description Some results of study for high-resolution spectra of Jupiter and Saturn atmospheres are presented. The spectral data are derived with the help of the coude echelle spectrometer installed on the 2-m telescope at the Terskol Observatory (the Northern Caucasus). The investigations are carried out with consideration for Raman light scattering. Calculations for molecular scattering effect in the atmospheres of giant planets are made for visible part of the spectrum. Wavelengths of Fraunhofer lines and their strongest ghosts caused by the rotational S(0), S(1), O(2) and the vibrational Q₁(1) transitions are used.
issn 0233-7665
url https://nasplib.isofts.kiev.ua/handle/123456789/79703
citation_txt Raman scattering effect in atmospheres of giant planets of the Solar System from high-resolution spectral data / Yu.G. Kuznyetsova, A.P. Vid'machenko // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 480-482. — Бібліогр.: 5 назв. — англ.
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