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Last modified
7/28/2009 2:38:14 PM
Creation date
4/16/2008 11:08:06 AM
Metadata
Fields
Template:
Weather Modification
Contract/Permit #
7-07-83-V0001
Title
Turbulant Diffusion Studies of Winter Storms Over the Sierra Nevada Mountains
Date
12/1/1981
Weather Modification - Doc Type
Report
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<br />. <br /> <br />. <br /> <br />5.7 <br /> <br />'. <br /> <br />5.8 <br /> <br />. <br /> <br />5.9 <br /> <br />. <br /> <br />5.10 <br /> <br />. <br /> <br />5.11 <br /> <br />. <br /> <br />e <br /> <br />5.12 <br /> <br />. <br /> <br />. <br /> <br />5.13 <br /> <br />. <br /> <br />l~e same as Fig. 5.4, except of true airspeed (TAB') <br /> <br />wind component. <br /> <br />Mean variances of longitudinal (u,2), lateral (v' 2), <br />2 <br />and ver t ica I (w' ) wind components, as we II as true <br />air$peed (TAB,2), are presented as a function of true <br />air~peed, on 23 June 1979 FTH case study. <br /> <br />Covariances (a), eddy dissipation rates (b), and air- <br /> <br />craft characteristic time scales (c) are presented as <br /> <br />a function of true airspeed, on 23 June 1979 FTH case <br /> <br />study . <br /> <br />A s;ensitivity test of the mean square particle dis- <br />pla!cement (0), of longitudinal and vertical wind com- <br /> <br />ponents, calculated according to the LTD model for <br />different values of <br /> <br />A ~chematic diagram of the Eulerian space-time depen- <br />dent autocorrelation function [RE(UT,T)] and the La- <br /> <br />grangian single-particle autocorrelation function <br />[RL(T)]. The moving, Eulerian-time dependent auto- <br /> <br />coli're la t ion func t ion, is presented ins ide the "enve- <br /> <br />IOJ?e ". <br /> <br />Schematic diagram of (a) families of Eulerian, space <br />dependent (Q) and space and time dependent (8) auto- <br /> <br />correlation functions in time domain, and (b) a single <br /> <br />space dependent Euler ian autocorre la t ion func t ion in <br /> <br />Ix <br /> <br />90 <br /> <br />91 <br /> <br />92 <br /> <br />94 <br /> <br />99 <br /> <br />space doma in. 100 <br /> <br />Power spectra (plotted as fE(f) versus f of longi- <br />
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