Show simple item record

contributor authorGilman, Peter A.
date accessioned2017-06-09T14:14:04Z
date available2017-06-09T14:14:04Z
date copyright1967/03/01
date issued1967
identifier issn0022-4928
identifier otherams-15294.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4150950
description abstractThe equations of Part I are approximated to represent a two-layer model. All the theorems for the continuous case are shown to hold in the two-layer case as well. In addition, bounds are placed on the phase velocities of neutral waves. The stability of purely baroclinic flow (no horizontal shear) in a uniform zonal magnetic field is then studied. The minimum vertical shear needed for instability no longer depends upon the ?-effect or the static stability, but rather is determined by the zonal field strength. Short waves are destabilized by the magnetic field, long waves stabilized. Unstable waves convert available potential energy into kinetic energy of the disturbances, part of which in turn is converted into disturbance magnetic energy. Nonmagnetic changes in the initial state are similar to those of Phillips. Perturbation vertical magnetic fields and a single-celled meridional (poloidal) field are produced.
publisherAmerican Meteorological Society
titleStability of Baroclinic Flows in a Zonal Magnetic Field: Part II
typeJournal Paper
journal volume24
journal issue2
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1967)024<0119:SOBFIA>2.0.CO;2
journal fristpage119
journal lastpage129
treeJournal of the Atmospheric Sciences:;1967:;Volume( 024 ):;issue: 002
contenttypeFulltext


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record