Title of article
Observation of a tilt of Titanʹs middle-atmospheric superrotation
Author/Authors
Achterberg، نويسنده , , Richard K. and Conrath، نويسنده , , Barney J. and Gierasch، نويسنده , , Peter J. and Flasar، نويسنده , , F. Michael and Nixon، نويسنده , , Conor A.، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2008
Pages
7
From page
549
To page
555
Abstract
Maps of isotherms on surfaces of constant pressure in Titanʹs middle atmosphere encircle the poles but show an offset, implying that the mean zonal flow has an axis of symmetry that is tilted relative to the spin axis of the solid body. The effect is seen in both hemispheres around a consistent axis. Periodogram analysis of the temperature field shows that wavenumber one, the signal corresponding to the spin tilt, is the strongest wave component. We conjecture that the tilt of the atmospheric spin is due to a feedback between the flow and the solar heating. The spin adjusts itself to align the spin equator with the direction toward the Sun, and thereby maximizes the efficiency with which the meridional circulation pumps angular momentum upward to generate superrotation.
Keywords
Titan , Atmospheresdynamics , Infrared observations , Atmospheresstructure
Journal title
Icarus
Serial Year
2008
Journal title
Icarus
Record number
2376418
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