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Can I read The dynamic meteorology of Titan on EtoBox?

The dynamic meteorology of Titan by F.M. Flasar is a Physics and Astronomy article available to read on EtoBox.

What is The dynamic meteorology of Titan about?

Current understanding of Titan|s atmo! spheric circulation and thermal structure is reviewed[ Knowledge of Titan|s zonal winds derives from tem! peratures retrieved from Voyager infrared measure! ments and geopotential heights retrieved from stellar occultation observations[ The inferred stratospheric winds are cyclostrophic\ like those of Venus[ Radiative response times are long in the lower troposphere\ but decline to values small compared to a season in the upper stratosphere[ Given Titan|s e}ective obliquity of 16>\ stratospheric temperatures and zonal winds should vary seasonally\ requiring a cross!equatorial Lagran! gian circulation to transport angular momentum and heat to maintain the thermal wind balance[ Atmo! spheric waves may play an important role in trans! porting and depositing angular momentum\ but they are as yet constrained by few observations[ General circulation models of Titan|s winds are still in their infancy\ but suggest much of the troposphere must be stably strati\_ed\ so that the cyclostrophic zonal winds aloft are isolated from surface drag[ The vertical struc! ture of temperature\ above the lowest 3 km\ is con! sistent with a radiatively balanced atmosp

Who reads The dynamic meteorology of Titan?

It is typically read by researchers, students, and practitioners in Physics and Astronomy.

Author
F.M. Flasar
Publisher
Elsevier Science; Elsevier ; Elsevier BV (ISSN 0032-0633)
Published
1998
Language
EN
Field
Physics and Astronomy (Physical Sciences)

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