On the axisymetric, steady state structure of the atmosphere
DOI:
https://doi.org/10.22201/igeof.00167169p.1974.14.2.985Palabras clave:
Atmósfera, Simetría axial, Estado estacionario, Calentamiento NewtonianoResumen
El estado estacionario y con simetría axial de la atmósfera se calcula usando un modelo cuasi geostrófico .de dos niveles. La función de calentamiento determinada por Fuenzalida (1973) ha sido usada y la circulación calculada de esta manera se compara con cálculos similares basados en varias parametrizaciones del calentamiento. Se presentan análisis detallados usando calentamiento newtoniano con consideraciones radiactivas únicamente e incorporando otros procesos físicos.
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WIIN-NIELSEN, A., and H. A. FUENZALIDA, 1974. On the simulation of the axisymmetric circulation of the atmosphere. Submitted for publication in Tellus. DOI: https://doi.org/10.1111/j.2153-3490.1975.tb01673.x
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Derechos de autor 1974 Geofísica Internacional
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