RESEARCHES OF LONG-TERM VARIATIONS IN URANUS AND NEPTUNE SPECTRA

Автор(и)

  • Yu. Kuznyetsova Main astronomical observatory of NAS of Ukraine, Україна
  • A. Vidmachenko Main astronomical observatory of NAS of Ukraine, Україна
  • O. Matsiaka Taras Shevchenko University of Kyiv, Україна
  • Y. Shliakhetskaya Main astronomical observatory of NAS of Ukraine, Україна
  • M. Yushkin Special astrophysical observatory of Russian Academy of Sciences, Російська Федерація
  • V. Krushevska Main astronomical observatory of NAS of Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2015.28.71130

Ключові слова:

Uranus, Neptune, giant planets, Raman light scattering, Fraunhofer lines H&K CaII

Анотація

The results of long-term spectral observations of Solar System giant planets Uranus and Neptune are presented here. Data were obtaining in period 2002-2012 at the peak Terskol Observatory (Northern Caucasus, Russia) using 2-meter Ritchey-Chretien telescope Zeiss-2000 with help coude echelle spectrograph and at the Special astrophysical observatory (SAO RAS, Northern Caucasus, Russia) with help 6-meter telescope using echelle spectrograph NES. Raman light scattering of solar photons by hydrogen molecules in the atmosphere spectra of Uranus and Neptune was registered in most powerful Fraunhofer lines H&K CaII as the "emission" details in center cores of these lines. Relative values of Raman scattering contribution for noted lines are estimated. Also, we have carried out long-term monitoring of Raman light scattering variations in cloudy surface spectra.

Посилання

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Опубліковано

2016-06-13

Номер

Том 28 № 2 (2015)

Розділ

Сонячна система

Ліцензія

Авторське право (c) 2015 Odessa Astronomical Publications

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Ця робота ліцензується відповідно до Creative Commons Attribution-NonCommercial 4.0 International License.

Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року