A study of vertical velocity distributions in the planetary boundary layer
โ Scribed by Frank Quintarelli
- Publisher
- Springer
- Year
- 1990
- Tongue
- English
- Weight
- 584 KB
- Volume
- 52
- Category
- Article
- ISSN
- 0006-8314
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โฆ Synopsis
Until recently, pollution dispersion models have made predictions on the basis that the pollutant concentration is Gaussian. Such is not the case for convective conditions where the observed vertical velocity distribution is skewed towards the updraught portion of the distribution. One recent dispersion mode1 assumes that the observed distribution can be synthesized by superimposing two Gaussians of appropriate means, variances and amplitudes.
In the current paper, two techniques for deriving the constituent distributions are investigated. The first technique is based on conditionally sampling the vertical velocity time series and partitioning the vertical velocity samples into two sets -one set recorded when the sensor was experiencing an updraught and the other when the sensor was experiencing a downdraught. The second method consists of fitting two Gaussian distributions to the observed data and adjusting these using an iterative procedure until a specified tolerance is achieved.
Both techniques give similar results which compare favourably with results obtained by other researchers. Assumptions, as well as advantages and disadvantages of each technique are also discussed.
๐ SIMILAR VOLUMES
Gravity waves associated with stably stratified layers were observed in the planetary boundary layer at two locations in France. Using an array of three monostatic Doppler acoustic sounders, the wave speeds and directions were found. A quantitative study of the waves has been performed to determine
The equations of motions are solved for concentric circular flow in the planetary boundary layer (PBL) under the assumption of K = 1' I&/& and gradient wind independent of radius r. The theoretical distribution of wind is obtained for r 2 300 km. Other parameters of the PBL are also calculated. Fina