US EditionTemporal Evolution Of Water Abundance In Saturn's Hot Vortex Of 2011-2013 - Astrobiology
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Temporal Evolution Of Water Abundance In Saturn's Hot Vortex Of 2011-2013 - Astrobiology
Water vapour is delivered to Saturn’s stratosphere by Enceladus’ plumes and subsequent diffusion in the planet system. It is expected to condense into a haze in the middle stratosphere. The hot stratospheric vortex (the `beacon’) that formed as an aftermath of Saturn’s Great Storm of 2010 significantly altered the temperature, composition, and circulation in Saturn’s […] The post Temporal Evolution Of Water Abundance In Saturn’s Hot Vortex Of 20…
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