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Numerical study of the nocturnal planetary boundary layer at low latitudes

机译:低纬度夜间行星边界层的数值研究

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A second order closure model is used to simulate the nighttime evolution of a Planetary Boundary Layer (PBL) over a continental area located in Ipero, Brazil,(23°5′S, 47°5′W). The numerical results show that the observed southerly nocturnal low level jet can be explained in terms of the meso-scale circulation induced by the slopped terrain. Two numerical simulation of the PBL was carried out using different mixing length expressions. One, based on the original master length scale proposed by Mellor & Yamada and, another using a new length scale proposed by Degrazia et al.[2], where the thermal stratification effect is explicitly include in mixing length. The results indicate that the mean field structure and the intensity of turbulence vary with different choice of mixing length scale, while the turbulence structure are less sensitive. In the Degrazia et al. [2] case the height of the PBL was smaller and the intensity of the low level jet was bigger and closer to the ground than in the Mellor & Yamada case. In both cases the height of the PBL coincides with the height of the low level jet and the top of the surface inversion.
机译:二阶封闭模型用于模拟位于巴西伊珀罗(23°5′S,47°5′W)的大陆区域上行星边界层(PBL)的夜间演化。数值结果表明,观察到的南风夜间低空急流可以用倾斜地形引起的中尺度环流来解释。使用不同的混合长度表达式对PBL进行了两个数值模拟。一种基于Mellor&Yamada提出的原始主长度标度,另一种基于Degrazia等人[2]提出的新的长度标度,其中热分层效应明确包括在混合长度中。结果表明,平均场结构和湍流强度随混合长度尺度的不同选择而变化,而湍流结构较不敏感。在Degrazia等。 [2]与Mellor&Yamada案例相比,PBL的高度较小,低空急流的强度更大且更接近地面。在这两种情况下,PBL的高度都与低位射流的高度和表面反转的顶部重合。

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