Jt. Bacmeister et al., STRATOSPHERIC HORIZONTAL WAVE-NUMBER SPECTRA OF WINDS, POTENTIAL TEMPERATURE, AND ATMOSPHERIC TRACERS OBSERVED BY HIGH-ALTITUDE AIRCRAFT, JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 101(D5), 1996, pp. 9441-9470
Horizontal wavenumber power spectra of vertical and horizontal wind ve
locities, potential temperatures, and ozone and N2O mixing ratios, as
measured in the mid-stratosphere during 73 ER-2 flights (altitude appr
oximate to 20 km) are presented. The velocity and potential temperatur
e spectra in the 100 to 1-km wavelength range deviate significantly fr
om the uniform -5/3 power law expected for the inverse energy-cascade
regime of two-dimensional turbulence and also for inertial-range, thre
e-dimensional turbulence. Instead, steeper spectra approximately consi
stent with a -3 power law are observed at horizontal scales smaller th
an 3 km for all velocity components as well as potential temperature.
Shallower spectra are observed at scales longer than 6 km. For horizon
tal velocity and potential temperature the spectral indices at longer
scales are between -1.5 and -2.0. For vertical velocity the spectrum a
t longer scales becomes flat. It is argued that the observed velocity
and potential temperature spectra are consistent with gravity waves. A
t smaller scales, the shapes are also superficially consistent with a
Lumley-Shur-Weinstock buoyant subrange of turbulence and/or nonlinear
gravity waves. Contemporaneous spectra of ozone and N2O mixing ratio i
n the 100 to 1-km wavelength range do conform to an approximately unif
orm -5/3 power law. It is argued that this may reflect interactions be
tween gravity wave air-parcel displacements and laminar or filamentary
structures in the trace gas mixing ratio field produced by enstrophy-
cascading two-dimensional turbulence.