Jw. Bergman et Ml. Salby, EQUATORIAL WAVE ACTIVITY DERIVED FROM FLUCTUATIONS IN OBSERVED CONVECTION, Journal of the atmospheric sciences, 51(24), 1994, pp. 3791-3806
The spectrum of equatorial wave activity propagating vertically into t
he stratosphere is calculated from high-resolution imagery of the glob
al convective pattern. Synoptic Global Cloud Imagery (GCI), constructe
d from six satellites simultaneously observing the earth, is used to d
iabatically force the linearized primitive equations. Having resolutio
n of 0.5 deg and 3 h, that imagery captures the dominant scales of org
anized convection, including several harmonics of the diurnal cycle. I
ts global coverage with high space-time resolution allows the GCI to r
epresent heating variability and dynamical behavior excited by it over
a wide range of scales. The dynamical response above the heating is e
valuated globally in terms of a space-time spectrum of Hough modes, on
e which includes planetary-scale Kelvin waves, Rossby waves, and gravi
ty waves down to the resolution of the GCI. The geopotential response,
which is indicative of temperature fluctuations observed by satellite
, is very red in frequency. Therefore, planetary-scale waves with peri
ods longer than two days dominate the spectrum of geopotential, while
high-frequency gravity waves make a comparatively small contribution.
Some 80% of the geopotential variance is accounted for by the Kelvin a
nd gravest-symmetric Rossby modes, while the Rossby-gravity mode is co
mparatively weak. In horizontal eddy motion, the excited wave spectrum
is still dominated by planetary-scale components. However, meridional
wind fluctuations associated with the Rossby-gravity mode have varian
ce comparable to that of zonal wind fluctuations associated with the K
elvin mode, even though the Rossby-gravity mode is nearly invisible in
the geopotential response. Estimates of tropospheric heating lead to
amplitudes and propagation characteristics that are broadly consistent
with satellite and radiosonde observations of wave activity in the lo
wer stratosphere. The space-time spectrum of EP flux is significantly
whiter than the response in either geopotential or motion. Gravity wav
es of small scale and high frequency carry a large fraction of the upw
ard flux. Although it dominates eastward variance of geopotential and
motion, the Kelvin mode carries only about 50% of the eastward EP flux
at phase speeds of 20-40 m s(-1) and only 35% of the total eastward B
ur transmitted to the stratosphere. The remainder is carried by the gr
avity wave spectrum, which carries nearly all of the westward flux at
phase speeds greater than 20 m s(-1). The gravity wave spectrum also c
ontributes significantly at phase speeds of 10-20 m s(-1) where only 2
5% of the flux is accounted for by zonal wavenumbers less than 20. The
broad nature of the gravity wave spectrum suggests its absorption at
critical levels will be distributed over a deep layer of the middle at
mosphere.