Seasonal Evolution of Saturn's Polar Temperatures and Composition
arXiv:1412.6416 · doi:10.1016/j.icarus.2014.11.022
Abstract
The seasonal evolution of Saturn's polar atmospheric temperatures and hydrocarbon composition is derived from a decade of Cassini Composite Infrared Spectrometer (CIRS) 7-16 m thermal infrared spectroscopy. We construct a near-continuous record of atmospheric variability poleward of 60 from northern winter/southern summer (2004, ) through the equinox (2009, ) to northern spring/southern autumn (2014, ). The hot tropospheric polar cyclones and the hexagonal shape of the north polar belt are both persistent features throughout the decade of observations. The hexagon vertices rotated westward by longitude between March 2007 and April 2013, confirming that they are not stationary in the Voyager-defined System III longitude system as previously thought. The extended region of south polar stratospheric emission has cooled dramatically poleward of the sharp temperature gradient near 75S, coinciding with a depletion in the abundances of acetylene and ethane, and suggestive of stratospheric upwelling with vertical wind speeds of mm/s. This is mirrored by a general warming of the northern polar stratosphere and an enhancement in acetylene and ethane abundances that appears to be most intense poleward of 75N, suggesting subsidence at mm/s. However, the sharp gradient in stratospheric emission expected to form near 75N by northern summer solstice (2017, ) has not yet been observed, so we continue to await the development of a northern summer stratospheric vortex. North polar minima in tropospheric and stratospheric temperatures were detected in 2008-2010 (lagging one season, or 6-8 years, behind winter solstice); south polar maxima appear to have occurred before the start of the Cassini observations (1-2 years after summer solstice). [Abridged]
arXiv commentPreprint of article accepted for publication in Icarus
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Cited by in corpus (15)
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