Observed propagation and structure of the 33-h atmospheric Kelvin wave

The structure of the 33-h Kelvin wave, a normal mode of the atmosphere, is examined in B-hourly station and NCEP-NCAR reanalysis data. Cross-spectral analysis of 6 yr (1993-98) of tropical station pressure data shows a peak i n coherence in a narrow frequency band centered near 0.74 cycles per day, c orresponding to a period of approximately 33 h. The phase angles are consis tent with an eastward-propagating zonal-wavenumber-1 structure, implying an equatorial phase speed of approximately 340 m s(-1). The global structure of the mode is revealed by empirical orthogonal function and regression ana lysis of 31 yr (1968-98) of reanalysis data. The horizontal structure shows a zonal-wavenumber-1 equatorial Kelvin wave with an equatorial trapping sc ale of approximately 340 lat. The vertical structure has zero phase change. The amplitude of the wave is approximately constant in the troposphere wit h an equatorial geopotential height perturbation of 0.9 m, and then increas es exponentially with height in the stratosphere. Cross-spectral analysis b etween the station and reanalysis data shows that the results from the two datasets are consistent. No evidence can be found for forcing of the wave b y deep tropical convection, which is is examined using a twice-daily outgoi ng longwave radiation dataset.