Mountain torque and angular momentum in barotropic planetary flows: equilibrium solutions
Mountain torque and angular momentum in barotropic planetary flows: equilibrium solutions
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正压行星流中的山扭矩和角动量:平衡解
DOI:
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发表时间:
1983
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影响因子:
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通讯作者:
J. Frederiksen
中科院分区:
文献类型:
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作者:
B. Sawford;J. Frederiksen
The climatic-mean-value of the total zonal relative angular momentum of the atmosphere in topographically forced inviscid barotropic models on a sphere is examined using the methods of equilibrium statistical mechanics. Models incorporating wave–wave interactions as well as simplified systems in which only wave–zonal-flow interactions are allowed are considered. It is shown analytically that for a given truncation the equilibrium state of the system does not depend on the presence of wave–wave interactions although the detailed evolution towards it does.
We interpret our results in terms of a generalization of the properties of the equilibrium solutions for unforced barotropic flow. For realistic resolution (with truncation wavenumber ° 15) most flows evolve towards an equilibrium with westward angular momentum, and the solutions are strongly dependent on the initial conditions. An important exception is the case when the flow initially has westward angular momentum, when the equilibrium state remains close to the initial state regardless of resolution. An upper bound on the climatic-mean-value of the solid-body rotation component of the flow is derived. In general, highly truncated systems are insensitive to the initial conditions and evolve towards a state in which the angular momentum is eastward and close to the upper bound.
Reasonable rescating of the global topography used has little influence on the climatic-mean angular momentum, but the case of no topography represents a singular limit in which angular momentum is conserved.