Corrected spectral dependence of the imaginary part of the refractive index of aerosol in Jupiter’s atmosphere in the short-wavelength spectral range
- Авторлар: Ovsak A.S.1, Morozhenko A.V.1
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Мекемелер:
- Main Astronomical Observatory
- Шығарылым: Том 33, № 5 (2017)
- Беттер: 239-244
- Бөлім: Dynamics and Physics of Bodies of the Solar System
- URL: https://ogarev-online.ru/0884-5913/article/view/177997
- DOI: https://doi.org/10.3103/S088459131705004X
- ID: 177997
Дәйексөз келтіру
Аннотация
To correctly determine the relative contribution of aerosol to the scattering properties of a gas–aerosol medium in the continuum, we propose a method that allows more reliable values of the imaginary part of the refractive index ni to be obtained for Jupiter’s atmosphere in the short-wavelength spectral range. We considered the measurement data on the spectral values of the geometric albedo of Jupiter acquired in 1993 and used the model of homogeneous spherical aerosol particles. The obtained values of ni are 0.00378, 0.00309, 0.00254, 0.00175, 0.00123, 0.00084, 0.00064, 0.00045, 0.00031, 0.00033, 0.00013, and 0.00008 at wavelengths λ = 320, 350, 375, 400, 420, 450, 470, 500, 520, 550, 606, and 631 nm, respectively.
Авторлар туралы
A. Ovsak
Main Astronomical Observatory
Хат алмасуға жауапты Автор.
Email: ovsak@mao.kiev.ua
Украина, Kyiv, 03143
A. Morozhenko
Main Astronomical Observatory
Email: ovsak@mao.kiev.ua
Украина, Kyiv, 03143
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