4.4 Article

On the Wave Spectrum Generated by Tropical Heating

Journal

JOURNAL OF THE ATMOSPHERIC SCIENCES
Volume 68, Issue 9, Pages 2042-2060

Publisher

AMER METEOROLOGICAL SOC
DOI: 10.1175/2011JAS3718.1

Keywords

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Funding

  1. NASA Atmospheric Composition: Aura Science Team [NNH08CD37C]
  2. NASA [NNH08CD34C]
  3. NSF [0121564]
  4. Div Atmospheric & Geospace Sciences
  5. Directorate For Geosciences [0121564] Funding Source: National Science Foundation

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Convective heating profiles are computed from one month of rainfall rate and cloud-top height measurements using global Tropical Rainfall Measuring Mission and infrared cloud-top products. Estimates of the tropical wave response to this heating and the mean flow forcing by the waves are calculated using linear and nonlinear models. With a spectral resolution up to zonal wavenumber 80 and frequency up to 4 cpd, the model produces 50%-70% of the zonal wind acceleration required to drive a quasi-biennial oscillation (QBO). The sensitivity of the wave spectrum to the assumed shape of the heating profile, to the mean wind and temperature structure of the tropical troposphere, and to the type of model used is also examined. The redness of the heating spectrum implies that the heating strongly projects onto Hough modes with small equivalent depth. Nonlinear models produce wave flux significantly smaller than linear models due to what appear to be dynamical processes that limit the wave amplitude. Both nonlinearity and mean winds in the lower stratosphere are effective in reducing the Rossby wave response to heating relative to the response in a linear model for a mean state at rest.

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