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NUMERICAL COMPUTATION OF PRESSURE GRADIENT FOR THE FLOW OF POWER-LAW FLUID IN ANNULUS WITH INNER CYLINDER EXECUTING A PLANETARY MOTION 被引量:1
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作者 CUI Hai-qing CAI Meng +1 位作者 ZHANG Shu-yun XIU De-yan 《Journal of Hydrodynamics》 SCIE EI CSCD 2009年第5期699-704,共6页
With the governing equations for the flow of the power-law fluid in annulus with the inner cylinder executing a planetary motion being transformed by using the undetermined coefficient method, the formula of pressure ... With the governing equations for the flow of the power-law fluid in annulus with the inner cylinder executing a planetary motion being transformed by using the undetermined coefficient method, the formula of pressure gradient for this flow under the given flow rate and the relevant numerical calculation method are given in this article. Through the experiments on the flow of Hydrolyzed Polyacrylamide (HPAM) aqueous solution which can be regarded as a power-law fluid, the calculated results of the pressure gradient values are compared with measured data, the mean relative error between them is smaller than 5%, which verifies the results presented in this article. 展开更多
关键词 power-law fluid planetary motion ANNULUS pressure gradient numerical calculation
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Effects of Turbulent Dispersion of Atmospheric Balance Motions of Planetary Boundary Layer 被引量:1
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作者 刘式适 黄伟 荣平平 《Advances in Atmospheric Sciences》 SCIE CAS CSCD 1992年第2期147-156,共10页
New Reynolds' mean momentum equations including both turbulent viscosity and dispersion are used to analyze atmospheric balance motions of the planetary boundary layer. It is pointed out that turbulent dispersion ... New Reynolds' mean momentum equations including both turbulent viscosity and dispersion are used to analyze atmospheric balance motions of the planetary boundary layer. It is pointed out that turbulent dispersion with r 0 will increase depth of Ekman layer, reduce wind velocity in Ekman layer and produce a more satisfactory Ekman spiral lines fit the observed wind hodograph. The wind profile in the surface layer including tur-bulent dispersion is still logarithmic but the von Karman constant k is replaced by k1 = 1 -2/k, the wind increasesa little more rapidly with height. 展开更多
关键词 Effects of Turbulent Dispersion of Atmospheric Balance motions of planetary Boundary Layer
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