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A proposed baroclinic wave test case for deep‐ and shallow‐atmosphere dynamical cores
Author(s) -
Ullrich Paul A.,
Melvin Thomas,
Jablonowski Christiane,
Staniforth Andrew
Publication year - 2013
Publication title -
quarterly journal of the royal meteorological society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.744
H-Index - 143
eISSN - 1477-870X
pISSN - 0035-9009
DOI - 10.1002/qj.2241
Subject(s) - baroclinity , hydrostatic equilibrium , instability , zonal flow (plasma) , atmosphere (unit) , geostrophic wind , geology , mechanics , atmospheric model , barotropic fluid , physics , meteorology , quantum mechanics , tokamak , plasma
Idealised studies of key dynamical features of the atmosphere provide insight into the behaviour of atmospheric models. A very important, well understood, aspect of midlatitude dynamics is baroclinic instability. This can be idealised by perturbing a vertically sheared basic state in geostrophic and hydrostatic balance. An unstable wave mode then results with exponential growth (due to linear dynamics) in time until, eventually, nonlinear effects dominate and the wave breaks. A new, unified, idealised baroclinic instability test case is proposed. This improves on previous ones in three ways. First, it is suitable for both deep‐ and shallow‐atmosphere models. Second, the constant surface pressure and zero surface geopotential of the basic state makes it particularly well‐suited for models employing a pressure‐ or height‐based vertical coordinate. Third, the wave triggering mechanism selectively perturbs the rotational component of the flow; this, together with a vertical tapering, significantly improves dynamic balance.