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141
Energy exchanges in Saturn's polar regions from Cassini observations: Eddy-zonal flow interactions
Published 2022“…Saturn's polar regions (polewards of ∼63° planetocentric latitude) are strongly dynamically active with zonal jets, polar cyclones and the intriguing north polar hexagon (NPH) wave. …”
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142
Impartment of spicy, fruity and herbal aromas from the Czech hop varieties of Ceres, Pluto and Saturn to beer
Published 2023-12-01“…Pluto has an intense fruity and herbal aroma, while Saturn has an intense fruity aroma with a milder citrus note. …”
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143
Earth-based Stellar Occultation Predictions for Jupiter, Saturn, Uranus, Neptune, Titan, and Triton: 2023–2050
Published 2023-01-01Subjects: Get full text
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144
MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert
Published 2023-01-01“…We analyze the MOA-2020-BLG-208 gravitational microlensing event and present the discovery and characterization of a new planet, MOA-2020-BLG-208Lb, with an estimated sub-Saturn mass. With a mass ratio $q={3.17}_{-0.26}^{+0.28}\times {10}^{-4}$ , the planet lies near the peak of the mass-ratio function derived by the MOA collaboration and near the edge of expected sample sensitivity. …”
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145
Parametrization of Horizontal and Vertical Transfers for the Street-Network Model MUNICH Using the CFD Model Code_Saturne
Published 2022-03-01“…This was developed based on a flow parametrization in a sparse vegetated canopy and adapted to street canyons using local-scale simulations performed with the CFD model Code_Saturne. CFD simulations were performed in a 2D infinite street canyon, and three streets of various aspect ratios ranging from <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>0.3</mn></mrow></semantics></math></inline-formula> to <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><mrow><mn>1.0</mn></mrow></semantics></math></inline-formula> were studied with different incoming wind directions. …”
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146
Semi-Analytical Search for Sun-Synchronous and Planet Synchronous Orbits around Jupiter, Saturn, Uranus and Neptune
Published 2022-07-01“…In this paper, some special orbits around Jupiter, Saturn, Uranus, and Neptune are discussed and analyzed. …”
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147
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148
Seasonal variations of temperature, acetylene and ethane in Saturn's atmosphere from 2005 to 2010, as observed by Cassini-CIRS
Published 2013“…Acetylene (C2H2) and ethane (C2H6) are by-products of complex photochemistry in the stratosphere of Saturn. Both hydrocarbons are important to the thermal balance of Saturn's stratosphere and serve as tracers of vertical motion in the lower stratosphere. …”
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149
CHANGES TO SATURN'S ZONAL-MEAN TROPOSPHERIC THERMAL STRUCTURE AFTER THE 2010-2011 NORTHERN HEMISPHERE STORM
Published 2014“…We use far-infrared (20-200 μm) data from the Composite Infrared Spectrometer on the Cassini spacecraft to determine the zonal-mean temperature and hydrogen para-fraction in Saturn's upper troposphere from observations taken before and after the large northern hemisphere storm in 2010-2011. …”
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150
HST hot-Jupiter transmission spectral survey: Clear skies for cool Saturn WASP-39b
Published 2016“…We present the Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) optical transmission spectroscopy of the cool Saturn-mass exoplanet WASP-39b from 0.29-1.025 μm, along with complementary transit observations from Spitzer IRAC at 3.6 and 4.5 μm. …”
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151
Saturn’s tropospheric particles phase function and spatial distribution from Cassini ISS 2010–11 observations
Published 2016Journal article -
152
Saturn's tropospheric particles phase function and spatial distribution from Cassini ISS 2010-11 observations
Published 2016Journal article -
153
The Manuscripts of <i>Solomon and Saturn</i>: CCCC 41, CCCC 422, BL Cotton Vitellius A.xv
Published 2022-04-01Subjects: “…<i>Solomon and Saturn</i>…”
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154
IMF dependence of Saturn's auroras: modelling study of HST and Cassini data from 12–15 February 2008
Published 2010-08-01“…Following earlier related studies of pre-orbit insertion data from January 2004 when Cassini was located ~ 1300 Saturn radii away from the planet, here we investigate the interval 12–15 February 2008, when UV images of Saturn's southern dayside aurora were obtained by the HST while the Cassini spacecraft measured the IMF in the solar wind just upstream of the dayside bow shock. …”
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155
Magnetospheric magnetic field modelling for the 2011 and 2012 HST Saturn aurora campaigns – implications for auroral source regions
Published 2014-06-01“…A unique set of images of Saturn's northern polar UV aurora was obtained by the Hubble Space Telescope in 2011 and 2012 at times when the Cassini spacecraft was located in the solar wind just upstream of Saturn's bow shock. …”
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156
Decision Making in City Planning: Processes of Visioning and Stakeholders Engagement and their Relation to Sustainable Land-Use in the SATURN Project
Published 2022-07-01“…The EIT Climate-KIC SATURN project deals with rural-urban territories, their landscapes and environmental challenges. …”
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157
Latitudinal variation of upper tropospheric NH3 on Saturn derived from Cassini/CIRS far-infrared measurements
Published 2012“…Ammonia (NH3) has been detected both on Saturn and Jupiter, and although its concentration and distribution has been well-studied on Jupiter, it has proven more difficult to do so on Saturn due to higher sensitivity requirements resulting from Saturn's lower atmospheric temperatures and the dominance of Saturn's phosphine which masks the ammonia signal. …”
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158
Hazes and clouds in a singular triple vortex in Saturn's atmosphere from HST/WFC3 multispectral imaging
Published 2019“…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. …”
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159
Deep winds beneath Saturn's upper clouds from a seasonal long-lived planetary-scale storm.
Published 2011“…Convective storms occur regularly in Saturn's atmosphere. Huge storms known as Great White Spots, which are ten times larger than the regular storms, are rarer and occur about once per Saturnian year (29.5 Earth years). …”
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160
Latitudinal variation of upper tropospheric NH3 on Saturn derived from Cassini/CIRS far-infrared measurements
Published 2012Journal article