首页> 外文期刊>Journal of the Atmospheric Sciences >On the Relationship between Inertial Instability, Poleward Momentum Surges, and Jet Intensifications near Midlatitude Cyclones
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On the Relationship between Inertial Instability, Poleward Momentum Surges, and Jet Intensifications near Midlatitude Cyclones

机译:中纬度气旋附近惯性不稳定性,极动量激增和急流激增之间的关系

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This study explores the role of inertial instability in poleward momentum surges and "flare ups'' of the subpolar jet near midlatitude cyclones. Two cases are simulated with the University of Wisconsin Nonhydrostatic Modeling System to investigate the mechanisms involved in jet accelerations downstream of quasi-stationary "digging troughs.'' Deep convection along the cold front leads to regions of inertial instability in the upper troposphere, which are intimately linked to jet accelerations. Terms in the zonal and meridional wind equations following the motion are evaluated for a selected air parcel within the inertially unstable region. A two-stage synoptic evolution is diagnosed, which is a characteristic signature of inertial instability. First, meridional flow accelerates following the motion, because of the subgeostrophic zonal flow and strong northward pressure gradient force (a statement of inertial instability). Second, supergeostrophic poleward flow leads to zonal acceleration and a jet flare-up. Inertial instability thus effectively displaces a westerly jet maximum poleward relative to inertially stable conditions. The structure of the poleward surge involves a distinctive "head'' of high angular momentum, with the region of inertial instability enclosing the jet maximum and a core of strongly negative potential vorticity inside the surge. Departures from angular momentum-conserving profiles during meridional displacement are interpreted in terms of the pressure gradient force and degree of inertial stability. Inertial instability reduces the resulting zonal wind profile relative to angular momentum conservation but provides a significant poleward displacement of the resulting zonal wind maximum.
机译:这项研究探索了惯性不稳定性在中纬度气旋附近的极向动量激增和子极射流“爆发”中的作用,并以威斯康星大学非静水模型系统为例,对两个案例进行了模拟,以研究准加速器下游射流加速的机制。沿冷锋的深对流会导致对流层上部的惯性不稳定区域,这些区域与射流加速度密切相关。运动后的纬向和经向风方程中的项将针对惯性不稳定区域内的选定空气包进行评估。诊断为两阶段天气演变,这是惯性不稳定性的特征。首先,由于亚地转带状纬向流和强大的北向压力梯度力(惯性不稳定性的陈述),子午流随着运动而加速。第二,超地转极流导致区域加速和射流爆发。惯性不稳定性因此有效地使西风射流的最大极移相对于惯性稳定条件。极地电涌的结构包括一个独特的高角动量“头部”,惯性不稳定性区域包围了射流的最大值,并且在电涌内部具有强烈的负电势涡旋核心,在子午线位移时偏离了角动量守恒分布相对于角动量守恒,惯性不稳定性降低了所产生的纬向风廓线,但产生了最大的纬向风向位移。

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