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 |
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| Datum: | 2005 |
| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | English |
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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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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. |
| work_keys_str_mv |
AT kuznyetsovayug ramanscatteringeffectinatmospheresofgiantplanetsofthesolarsystemfromhighresolutionspectraldata AT vidmachenkoap ramanscatteringeffectinatmospheresofgiantplanetsofthesolarsystemfromhighresolutionspectraldata |
| first_indexed |
2025-12-02T09:40:18Z |
| last_indexed |
2025-12-02T09:40:18Z |
| _version_ |
1850862127448850432 |