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...

Full description

Saved in:
Bibliographic Details
Published in:Кинематика и физика небесных тел
Date:2005
Main Authors: Kuznyetsova, Yu.G., Vid'machenko, A.P.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2005
Subjects:
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/79703
Tags: Add Tag
No Tags, Be the first to tag this record!
Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this: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.

Institution

Digital Library of Periodicals of National Academy of Sciences of Ukraine
_version_ 1862659575908401152
author Kuznyetsova, Yu.G.
Vid'machenko, A.P.
author_facet Kuznyetsova, Yu.G.
Vid'machenko, A.P.
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.
collection DSpace DC
container_title Кинематика и физика небесных тел
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.
first_indexed 2025-12-02T09:40:18Z
format Article
fulltext
id nasplib_isofts_kiev_ua-123456789-79703
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
issn 0233-7665
language English
last_indexed 2025-12-02T09:40:18Z
publishDate 2005
publisher Головна астрономічна обсерваторія НАН України
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
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 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_short 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
topic MS5: Dynamics and Physics of Solar System Bodies
topic_facet MS5: Dynamics and Physics of Solar System Bodies
url https://nasplib.isofts.kiev.ua/handle/123456789/79703
work_keys_str_mv AT kuznyetsovayug ramanscatteringeffectinatmospheresofgiantplanetsofthesolarsystemfromhighresolutionspectraldata
AT vidmachenkoap ramanscatteringeffectinatmospheresofgiantplanetsofthesolarsystemfromhighresolutionspectraldata