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Geophysical research letters, v.43 no.14, 2016년, pp.7774 - 7780
Liu, Junjun (California Institute of Technology, Pasadena, California, USA) , Schneider, Tapio (California Institute of Technology, Pasadena, California, USA)
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AbstractEarth and Titan exhibit contrasting atmospheric responses to orbital precession. On Earth, most (water) precipitation falls in low latitudes, and precipitation is enhanced in a hemisphere when perihelion occurs in that hemisphere's summer. On Titan, most (methane) precipitation falls in high...
Key PointsEarth and Titan exhibit contrasting precession responses because of their different rotation ratesFor Titan, length of summer controls hemispheric asymmetries of the precipitation responseFor Earth, maximum insolation controls hemispheric asymmetries of the precipitation response
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