Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging

In this paper we present a study of the vertical haze and cloud structure over a triple vortex in Saturn's atmosphere in the planetographic latitude range 55°N-69°N (del Río-Gaztelurrutia et al., 2018) using HST/WFC3 multispectral imaging. The observations were taken during 29–30 June and 1 Jul...

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Автори: Sanz-Requena, J, Perez-Hoyos, S, Sanchez-Lavega, A, Del Rio-Gaztelurrutia, T, Irwin, P
Формат: Journal article
Мова:English
Опубліковано: Elsevier 2019
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author Sanz-Requena, J
Perez-Hoyos, S
Sanchez-Lavega, A
Del Rio-Gaztelurrutia, T
Irwin, P
author_facet Sanz-Requena, J
Perez-Hoyos, S
Sanchez-Lavega, A
Del Rio-Gaztelurrutia, T
Irwin, P
author_sort Sanz-Requena, J
collection OXFORD
description In this paper we present a study of the vertical haze and cloud structure over a triple vortex in Saturn's atmosphere in the planetographic latitude range 55°N-69°N (del Río-Gaztelurrutia et al., 2018) using HST/WFC3 multispectral imaging. The observations were taken during 29–30 June and 1 July 2015 at ten different filters covering spectral range from the 225 nm to 937 nm, including the deep methane band at 889 nm. Absolute reflectivity measurements of this region at all wavelengths and under a number of illumination and observation geometries are fitted with the values produced by a radiative transfer model. Most of the reflectivity variations in this wavelength range can be attributed to changes in the tropospheric haze. The anticyclones are optically thicker (τ ~25 vs ~10), more vertically extended (~3 gas scale heights vs ~2) and their bases are located deeper in the atmosphere (550 mbar vs 500 mbar) than the cyclone.
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spelling oxford-uuid:23fb70db-a6c5-4626-84c3-ba0cce06d5f72022-03-26T11:47:20ZHazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imagingJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:23fb70db-a6c5-4626-84c3-ba0cce06d5f7EnglishSymplectic Elements at OxfordElsevier2019Sanz-Requena, JPerez-Hoyos, SSanchez-Lavega, ADel Rio-Gaztelurrutia, TIrwin, PIn this paper we present a study of the vertical haze and cloud structure over a triple vortex in Saturn's atmosphere in the planetographic latitude range 55°N-69°N (del Río-Gaztelurrutia et al., 2018) using HST/WFC3 multispectral imaging. The observations were taken during 29–30 June and 1 July 2015 at ten different filters covering spectral range from the 225 nm to 937 nm, including the deep methane band at 889 nm. Absolute reflectivity measurements of this region at all wavelengths and under a number of illumination and observation geometries are fitted with the values produced by a radiative transfer model. Most of the reflectivity variations in this wavelength range can be attributed to changes in the tropospheric haze. The anticyclones are optically thicker (τ ~25 vs ~10), more vertically extended (~3 gas scale heights vs ~2) and their bases are located deeper in the atmosphere (550 mbar vs 500 mbar) than the cyclone.
spellingShingle Sanz-Requena, J
Perez-Hoyos, S
Sanchez-Lavega, A
Del Rio-Gaztelurrutia, T
Irwin, P
Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
title Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
title_full Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
title_fullStr Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
title_full_unstemmed Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
title_short Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
title_sort hazes and clouds in a singular triple vortex in saturn s atmosphere from hst wfc3 multispectral imaging
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