Cassini Imaging Science Subsystem observations of Titan’s south polar cloud

•We document the shape, texture, color, and altitude of Titan’s S. polar cloud.•The altitude of the cloud is 300±15km.•The cloud rotates in 8h about a point offset from Titan’s spin axis.•Cloud texture suggests a condensate (HCN) in an open-cell convection pattern.•Cloud optical thickness is ∼1.5. I...

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Bibliographic Details
Published in:Icarus (New York, N.Y. 1962) N.Y. 1962), 2016-05, Vol.270, p.399-408
Main Authors: West, R.A., Del Genio, A.D., Barbara, J.M., Toledo, D., Lavvas, P., Rannou, P., Turtle, E.P., Perry, J.
Format: Article
Language:English
Subjects:
Cassini mission
Clouds
Imaging
Saturn satellites
Surface layer
Texture
Titan
Titan, atmosphere
Titan, clouds
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Summary:•We document the shape, texture, color, and altitude of Titan’s S. polar cloud.•The altitude of the cloud is 300±15km.•The cloud rotates in 8h about a point offset from Titan’s spin axis.•Cloud texture suggests a condensate (HCN) in an open-cell convection pattern.•Cloud optical thickness is ∼1.5. In May of 2012 images of Titan obtained by the Cassini Imaging Science Subsystem (ISS) showed a newly-formed cloud patch near the southern pole. The cloud has unusual morphology and texture suggesting that it is formed by condensation at an altitude much higher than expected for any of the known organics in Titan’s atmosphere. We measured the altitude to be 300±10km from images when the feature was on the limb. Limb images suggest that the initial stages of the formation began in late 2011. It was just visible in images obtained in 2014 but is not expected to be visible in the future due to enveloping darkness as the season progresses. The feature has a slightly different color than the surrounding haze. Its optical thickness is near 2 at 889nm wavelength and the particle imaginary refractive index must be less than 5×10−4 at that wavelength. Wind vectors derived from a time series show that it is rotating about a center offset by 4.5° from Titan’s solid-body spin axis, consistent with that found from the temperature field by Achterberg et al. (Achterberg, R.K., Conrath, B.J., Gierasch, P.J., Flasar, F.M., Nixon, C.A. [2008a]. Icarus 197, 549–555) and subsequent measurements. The feature rotates at an angular velocity near the rate expected for transport of angular momentum from the low latitudes to the pole. The clumpy texture of the feature resembles that of terrestrial cloud fields undergoing open cell convection, an unusual configuration initiated by downwelling.
ISSN:0019-1035
1090-2643
DOI:10.1016/j.icarus.2014.11.038