Numerical experiments on planetary meridional temperature gradients contrary to radiational forcing

Details Numerical experiments on planetary meridional temperature gradients contrary to radiational forcing Numerical experiments on planetary meridional temperature gradients contrary to radiational forcing

Dec 1965

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965papge..62..173p&link_type=abstract

Pure and Applied Geophysics PAGEOPH, Volume 62, Issue 1, pp.173-190

Physics

Geophysics

2

Scientific paper

The existence of the phenomenon that the temperature in certain layers of the earth's atmosphere is higher at the pole than at the equator is considered as a general problem in planetary fluid dynamics. In a highly simplified model the solution of the problem depends upon a group of non-dimensional parameters. Taking the parameters of the earth's atmosphere as an example, numerical experiments were performed to study the nature of such a meridional counterradiational-heating temperature gradient and the dependence of it on the vertical variation of meridional differential radiation. Some general inferences were drawn from the experiments.

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