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Multi-platform Observations Characterizing the Afternoon-to-Evening Transition of the Planetary Boundary Layer in Northern Alabama, USA

机译:表征美国阿拉巴马州北部行星边界层从下午到晚上过渡的多平台观测

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Observations from the University of Alabama in Huntsville campus and ground-based scanning radar for over 140 total spring, summer, and autumn cases are studied to contribute to the relative scarcity of long-term datasets documenting the afternoon-to-evening transition of the planetary boundary layer. A sunset relative frame of reference is employed, focusing on the period 3 h before to 2 h after astronomical sunset, and several findings are consistent with previous investigations. Fluctuating components of wind and temperature computed from nearly collocated surface, Doppler wind profiler, and vertically pointing Doppler lidar measurements show a consistent decline as turbulence intensity diminishes through the transition. When normalized by their initial values, a pattern emerges: temperature variances decline slowly at first then quite abruptly after about 90 min before sunset. After the temperature variances begin to wane, vertical velocity fluctuations decrease, and the rate of their decay increases as vigorous thermal structures diminish. The fastest decline of the horizontal wind variance occurs after an accelerated vertical wind variance decrease, and the horizontal wind fluctuations display the slowest rate of decrease among these quantities. Near-surface humidity measurements show increases in mean water vapour mixing ratio as a steady rise generally beginning about 80 min prior to sunset. Composites of mean lidar vertical motion show final convective-type towers of upward motion occur about an hour before sunset and are coherent through 800 m (all heights a.g.l.). Lidar vertical motion variance at 195 m decreases by more than an order of magnitude approaching sunset, then remains below 0.01 m s for the rest of the studied time frame. Subtle, but steady, increases in both horizontal wind speed and radar-derived horizontal wind convergence above the surface layer (at 300 m) span the entire 5-h time frame. While the convergence results show a broad range, an increase in the mean is clear and found to be statistically significant. Implications for possible transition-effect enhancements to pre-existing low-level convergence areas are briefly noted.
机译:来自阿拉巴马大学亨茨维尔分校的观测和地面扫描雷达对总共140例春季,夏季和秋季的案例进行了研究,这有助于记录行星从下午到晚上过渡的长期数据集的相对稀缺性边界层。采用日落的相对参照系,重点是天文日落之前3小时到之后2小时,并且一些发现与以前的研究一致。从几乎并置的表面,多普勒风廓线仪和垂直指向的多普勒激光雷达测量值计算出的风和温度的波动分量显示,随着湍流强度在过渡过程中的减小,其持续下降。当用它们的初始值归一化时,会出现一个模式:温度变化首先缓慢下降,然后在日落前约90分钟后突然下降。温度变化开始减弱后,垂直的速度波动会减小,并且随着剧烈的热结构减弱,其衰减速率也会增加。在垂直风速方差加速减小之后,水平风速方差的下降最快,而水平风速方差在这些量中的下降速度最慢。近地表湿度测量结果显示,平均水蒸气混合比随着稳定上升而增加,通常在日落之前约80分钟开始。平均激光雷达垂直运动的合成物显示出最终的对流式向上运动的塔楼发生在日落前约一个小时,并且贯穿800 m(所有高度均为a)。激光雷达在195 m处的垂直运动方差在接近日落时减少了一个数量级以上,然后在其余研究时间范围内保持在0.01 m s以下。在整个5小时的时间范围内,表层上方(300 m)的水平风速和雷达衍生的水平风收敛都微妙而稳定地增加。虽然收敛结果显示范围很广,但均值的增加很明显,并且在统计上是显着的。简要指出了对可能存在的过渡效果增强的影响。

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