Deep zonal winds can result from shallow driving in a giant-planet atmosphere

Adam Showman, Peter J. Gierasch, Yuan Lian

Research output: Contribution to journalArticle

29 Citations (Scopus)

Abstract

A simple model shows that acceleration of Jupiter and Saturn's multiple jets at altitudes confined near the top of the adiabatic region (e.g., at a few bars pressure) can produce jets that penetrate deeply into the molecular envelope. This result disproves the common assertion that jet acceleration near the outer margin can only produce zonal winds that are confined to these outer layers.

Original languageEnglish (US)
Pages (from-to)513-526
Number of pages14
JournalIcarus
Volume182
Issue number2
DOIs
StatePublished - Jun 2006

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zonal wind
planets
planet
atmospheres
atmosphere
Saturn
Jupiter (planet)
Jupiter
margins
envelopes

Keywords

  • atmosphere
  • Atmospheres
  • dynamics
  • Jupiter

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Deep zonal winds can result from shallow driving in a giant-planet atmosphere. / Showman, Adam; Gierasch, Peter J.; Lian, Yuan.

In: Icarus, Vol. 182, No. 2, 06.2006, p. 513-526.

Research output: Contribution to journalArticle

Showman, Adam ; Gierasch, Peter J. ; Lian, Yuan. / Deep zonal winds can result from shallow driving in a giant-planet atmosphere. In: Icarus. 2006 ; Vol. 182, No. 2. pp. 513-526.
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