Show simple item record

contributor authorShapiro, Alan
contributor authorKanak, Katharine M.
date accessioned2017-06-09T14:37:47Z
date available2017-06-09T14:37:47Z
date copyright2002/07/01
date issued2002
identifier issn0022-4928
identifier otherams-23148.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4159677
description abstractThe rise of an isolated dry thermal bubble in a quiescent unstratified environment is a prototypical natural convective flow. This study considers the rise of an isolated dry thermal bubble of ellipsoidal shape (elliptical in both horizontal and vertical cross sections). The azimuthal asymmetry of the bubble allows the vorticity tilting mechanism to operate without an environmental wind. The dry Boussinesq equations of motion are solved analytically as a Taylor series in time for the early time behavior of the bubble (involving derivatives of up to the third order in time). The analytic results are supplemented with numerical simulations to examine the longer-time behavior. The first nonzero term in the Taylor expansion for the vertical vorticity is a third-order term, and appears as a four-leaf clover pattern with lobes of alternating sign. The horizontal flow associated with this vorticity pattern first appears as a sheared stagnation point-type flow, but eventually organizes into vertical vortices that fill the bubble. The vortices induce large structural changes to the bubble and eventually reverse the sense of the azimuthal asymmetry.
publisherAmerican Meteorological Society
titleVortex Formation in Ellipsoidal Thermal Bubbles
typeJournal Paper
journal volume59
journal issue14
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(2002)059<2253:VFIETB>2.0.CO;2
journal fristpage2253
journal lastpage2269
treeJournal of the Atmospheric Sciences:;2002:;Volume( 059 ):;issue: 014
contenttypeFulltext


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record