The fully developed superrotation simulated by a general circulation model of a Venus-like atmosphere

Masaru Yamamoto, Masaaki Takahashi

Research output: Contribution to journalArticle

85 Citations (Scopus)

Abstract

Formation and maintenance of the fully developed superrotation in the Venus atmosphere are investigated by using a Center for Climate System Research/National Institute for Environmental Study (CCSR/NIES) Venuslike atmospheric general circulation model. Under the condition that zonally uniform solar heating is used, the meridional circulation is dominated by a single cell in a whole atmosphere, and the superrotation with velocities faster than 100 m s-1 is formed near 60-km altitude. The meridional circulation effectively pumps up angular momentum from the lower to the middle atmosphere. Then the angular momentum is transported by poleward flows of the meridional circulation, and a part of the transported momentum is returned back to the low-latitudinal regions by waves. As a result, the simulated superrotation is formed by the Gierasch mechanism. Equatorward angular momentum flux required in the Gierasch mechanism is caused by not only barotropic waves but also various waves. Rossby, mixed Rossby-gravity, and gravity waves transport the angular momentum equatorward. Although vertically propagating gravity waves decelerate the superrotation above 70 km, the fully developed superrotation can be maintained in the cloud layer (45-70 km).

Original languageEnglish
Pages (from-to)561-573
Number of pages13
JournalJournal of the Atmospheric Sciences
Volume60
Issue number3
DOIs
Publication statusPublished - Feb 1 2003
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Atmospheric Science

Fingerprint Dive into the research topics of 'The fully developed superrotation simulated by a general circulation model of a Venus-like atmosphere'. Together they form a unique fingerprint.

Cite this