A comparison of vertical velocity variance measurements from wind profiling radars and sonic anemometers

Observations of turbulence in the planetary boundary layer are critical for developing and evaluating boundary layer parameterizations in mesoscale numerical weather prediction models. These observations, however, are expensive and rarely profile the entire boundary layer. Using optimized configurat...

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Bibliographic Details
Main Authors: K. McCaffrey, L. Bianco, P. Johnston, J. M. Wilczak
Format: Article
Language:English
Published: Copernicus Publications 2017-03-01
Series:Atmospheric Measurement Techniques
Online Access:http://www.atmos-meas-tech.net/10/999/2017/amt-10-999-2017.pdf
Description
Summary:Observations of turbulence in the planetary boundary layer are critical for developing and evaluating boundary layer parameterizations in mesoscale numerical weather prediction models. These observations, however, are expensive and rarely profile the entire boundary layer. Using optimized configurations for 449 and 915 MHz wind profiling radars during the eXperimental Planetary boundary layer Instrumentation Assessment (XPIA), improvements have been made to the historical methods of measuring vertical velocity variance through the time series of vertical velocity, as well as the Doppler spectral width. Using six heights of sonic anemometers mounted on a 300 m tower, correlations of up to <i>R</i><sup>2</sup> = 0. 74 are seen in measurements of the large-scale variances from the radar time series and <i>R</i><sup>2</sup> = 0. 79 in measurements of small-scale variance from radar spectral widths. The total variance, measured as the sum of the small and large scales, agrees well with sonic anemometers, with <i>R</i><sup>2</sup> = 0. 79. Correlation is higher in daytime convective boundary layers than nighttime stable conditions when turbulence levels are smaller. With the good agreement with the in situ measurements, highly resolved profiles up to 2 km can be accurately observed from the 449 MHz radar and 1 km from the 915 MHz radar. This optimized configuration will provide unique observations for the verification and improvement to boundary layer parameterizations in mesoscale models.
ISSN:1867-1381
1867-8548