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Thermodynamic and Turbulence Characteristics of the Southern Great Plains Nocturnal Boundary Layer Under Differing Turbulent Regimes

机译:不同湍流条件下大平原南部夜间边界层的热力学和湍流特征

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The nocturnal stable boundary layer (SBL) can generally be classified into the weakly stable boundary layer (wSBL) and very stable boundary layer (vSBL). Within the wSBL, turbulence is relatively continuous, whereas in the vSBL, turbulence is intermittent and not well characterized. Differentiating characteristics of each type of SBL are still unknown. Herein, thermodynamic and kinematic data collected by a suite of instruments in north central Oklahoma in autumn 2012 are analyzed to better understand both SBL regimes and their differentiating characteristics. Many low-level jets were observed during the experiment, as it took place near a climatological maximum. A threshold wind speed, above which bulk shear-generated turbulence develops, is found to exist up to 300 m. The threshold wind speed must also be exceeded at lower heights (down to the surface) in order for strong turbulence to develop. Composite profiles, which are normalized using low-level jet scaling, of potential temperature, wind speed, vertical velocity variance, and the third-order moment of vertical velocity () are produced for weak and moderate/strong turbulence regimes, which exhibit features of the vSBL and wSBL, respectively. Within the wSBL, turbulence is generated at the surface and transported upward. In the vSBL, values of vertical velocity variance are small throughout the entire boundary layer, likely due to the fact that a strong surface inversion typically forms after sunset. The temperature profile tends to be approximately isothermal in the lowest portions of the wSBL, and it did not substantially change over the night. Within both types of SBL, stability in the residual layer tends to increase as the night progresses. It is thought that this stability increase is due to differential warm air advection, which frequently occurs in the southern Great Plains when southerly low-level jets and a typical north-south temperature gradient are present. Differential radiative flux divergence also contributes to this increase in stability.
机译:夜间稳定边界层(SBL)通常可以分为弱稳定边界层(wSBL)和非常稳定边界层(vSBL)。在wSBL中,湍流是相对连续的,而在vSBL中,湍流是间歇性的并且没有很好的特征。每种SBL的区别特征仍然未知。本文对2012年秋季在俄克拉荷马州中北部的一套仪器收集的热力学和运动学数据进行了分析,以更好地了解SBL体制及其区分特征。在实验过程中观察到许多低空急流,因为它是在气候最大值附近发生的。已发现存在一个阈值风速,在该阈值风速以下会出现大块剪切产生的湍流,最高可达300 m。在较低的高度(向下到达地面)也必须超过阈值风速,以形成强烈的湍流。对于弱和中/强湍流区,使用低速射流定标对潜在温度,风速,垂直速度方差和垂直速度的三次矩()进行了归一化的复合轮廓产生了vSBL和wSBL。在wSBL内,湍流在表面产生并向上传输。在vSBL中,垂直速度方差的值在整个边界层都很小,这可能是由于通常在日落之后会形成很强的表面反转这一事实。在wSBL的最低部分,温度曲线趋于近似等温,并且在一夜之间基本上没有变化。在两种类型的SBL中,残留层的稳定性都会随着夜晚的进行而增加。可以认为,这种稳定性的提高是由于不同的暖空气对流引起的,当在南风低空急流和典型的南北向温度梯度出现时,在大平原南部经常发生。差分辐射通量散度也有助于增加稳定性。

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