Tidal theory with Newtonian cooling

作者: Richard S. Lindzen , Donald J. McKenzie

DOI: 10.1007/BF00875315

关键词:

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

参考文章(5)
C. Prabhakara, Joseph S. Hogan, Ozone and carbon dioxide heating in the martian atmosphere. Journal of the Atmospheric Sciences. ,vol. 22, pp. 97- 109 ,(1965) , 10.1175/1520-0469(1965)022<0097:OACDHI>2.0.CO;2
The Excitation of Atmospheric Oscillations Proceedings of The Royal Society A: Mathematical, Physical and Engineering Sciences. ,vol. 274, pp. 91- 121 ,(1963) , 10.1098/RSPA.1963.0116
Richard S. Lindzen, On the asymmetric diurnal tide Pure and Applied Geophysics. ,vol. 62, pp. 142- 147 ,(1965) , 10.1007/BF00875296
R. S. Lindzen, Thermally driven diurnal tide in the atmosphere Quarterly Journal of the Royal Meteorological Society. ,vol. 93, pp. 18- 42 ,(1967) , 10.1002/QJ.49709339503