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- W2024673804 abstract "Temporal spectra and cross-spectra of the three turbulent wind components for meso-synoptic scales at 250 m vertical intervals in the planetary boundary layer are presented. The data were derived from hourly simultaneous balloon ascents from a 5-point grid at Hay, New South Wales, Australia (lat. 34 ½S), during the Wangara expedition. The spectra indicate a meso-scale gap for u (eastward component of wind) and v (northward component). The computed w-spectra suggest that no marked gap is present. For periods less than 1 day the u- and v-spectra, with a correction applied for high frequency noise, fall off approximately as n−2·6, where n is the frequency, and this result appears to be invariant with height within and just above the planetary boundary layer. The corrected w-spectra exhibit n−1 dependency in this frequency range. The uv, uw, and vw cospectra also show only small contributions on the meso-scale (periods less than a day) compared to the synoptic scale, indicating that meso-scale motions may not have to be explicitly modelled in atmospheric general circulation models. An inertial peak is found for u and v but the w-spectra show a diurnal peak. The phase angles showed that u and v were in approximate quadrature at the inertial frequency, demonstrating the existence of the inertial cycle. Tests for horizontally two-dimensional isotropy indicated that the turbulence did not obey this simplification." @default.
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- W2024673804 date "1973-01-01" @default.
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- W2024673804 title "Time spectra and cross-spectra of kinetic energy in the planetary boundary layer" @default.
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- W2024673804 doi "https://doi.org/10.1002/qj.49709941912" @default.
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