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pure and applied geophysics

, Volume 66, Issue 1, pp 90–96 | Cite as

Tidal theory with Newtonian cooling

  • Richard S. Lindzen
  • Donald J. McKenzie
Article

Summary

Processes representable by Newtonian cooling models are found to be of importance for tides in various planetary atmospheres. The equations of tidal theory are, therefore, rederived to include a rather general Newtonian cooling, and some of the effects of this inclusion are investigated.

Keywords

Atmosphere Planetary Atmosphere Cool Model Newtonian Cool Tidal Theory 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. [1]
    M. Siebert,Atmospheric tides, Advances in Geophysics (1961), 105.Google Scholar
  2. [2]
    R. S. Lindzen,Thermally driven diurnal tide in the atmosphere, Submitted to Quarterly Jour. Roy. Met. Soc. (1966).Google Scholar
  3. [3]
    C. L. Pekeris andZ. Alterman,A method of solving nonlinear equations of atmospheric tides with applications to an atmosphere of constant temperature (The atmosphere and the sea in motion, Rockefeller Institute Press, New York 1959).Google Scholar
  4. [4]
    M. Yanowitch,The effect of viscosity on gravity waves and the upper boundary condition, NCAR manuscript No.147 (1966).Google Scholar
  5. [5]
    S. T. Butler andK. A. Small,The excitation of atmospheric oscillations, Proc. Roy. Soc. [A],274 (1963), 91.Google Scholar
  6. [6]
    R. S. Lindzen andR. M. Goody,Radiative and photochemical processes in mesospheric dynamics. Part I, Models for radiative and photochemical processes, Jour. Atmos. Sci.22 (1965), 341.Google Scholar
  7. [7]
    C. Prabhakara andJ. S. Hogan,Ozone and carbon dioxide heating in the martian atmosphere, Jour. Atmos. Sci.22 (1965), 97.Google Scholar
  8. [8]
    C. Leovy andY. H. Mintz,A numerical general circulation experiment for the atmosphere of mars, RAND report (1966), available from RAND Corp., Santa Monica, California, USA.Google Scholar
  9. [9]
    R. S. Lindzen,On the asymmetric diurnal tide, Pageoph62/III (1965), 142.Google Scholar
  10. [10]
    M. V. Wilkes,Oscillations of the earth's atmosphere (Cambridge University Press, 1949).Google Scholar

Copyright information

© Birkh#x00E4;user Verlag 1967

Authors and Affiliations

  • Richard S. Lindzen
    • 1
  • Donald J. McKenzie
    • 2
  1. 1.National Center for Atmospheric ResearchBoulderUSA
  2. 2.University of WashingtonSeattleUSA

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