کد مقاله کد نشریه سال انتشار مقاله انگلیسی نسخه تمام متن
1775801 1021207 2008 7 صفحه PDF دانلود رایگان
عنوان انگلیسی مقاله ISI
Observation of a tilt of Titan's middle-atmospheric superrotation
موضوعات مرتبط
مهندسی و علوم پایه علوم زمین و سیارات علوم فضا و نجوم
پیش نمایش صفحه اول مقاله
Observation of a tilt of Titan's middle-atmospheric superrotation
چکیده انگلیسی

Maps of isotherms on surfaces of constant pressure in Titan's 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.

ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Icarus - Volume 197, Issue 2, October 2008, Pages 549–555
نویسندگان
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