Stability of Convection between the Day and Night Sides on the Rotating Sphere
Author:
Affiliation:
1. Department of Earth and Planetary Physics, University of Tokyo
Publisher
Meteorological Society of Japan
Subject
Atmospheric Science
Link
https://www.jstage.jst.go.jp/article/jmsj1965/78/2/78_2_181/_pdf
Reference7 articles.
1. Gill, A. E., 1980: Some simple solutions for heat-induced tropical circulation. Quart. J. Roy. Meteor. Soc., 106, 447-462.
2. Itoh, H., 1993: Methods for obtaining stationary solutions of the primitive equation model and stationary and periodic solutions of the quasi-geostrophic model. J. Meteor. Soc. Japan, 71, 305-319.
3. Longuet-Higgins, M. S., 1968: The eigenfunctions of Laplace's tidal equations over a sphere. Phil. Trans. Roy. Soc. London, A262, 511-607.
4. Matsuda, Y. and T. Kato, 1987: The linear response of a global atmosphere to tropical heating-effect of planetary rotation. J. Meteor. Soc. Japan, 65, 819-842.
5. Schubert, G. and J. A. Whitehead, 1967: Moving flame experiment with liquid mercury: Possible implications for the Venus atmosphere. Science, 163, 71-72.
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1. Three-Dimensional Structures of Thermal Tides Simulated by a Venus GCM;Journal of Geophysical Research: Planets;2018-02
2. Effects of thermal tides on the Venus atmospheric superrotation;Journal of Geophysical Research;2007-05-09
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