首页> 外文期刊>Journal of the Atmospheric Sciences >Storm-Track Shifts under Climate Change: Toward a Mechanistic Understanding Using Baroclinic Mean Available Potential Energy
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Storm-Track Shifts under Climate Change: Toward a Mechanistic Understanding Using Baroclinic Mean Available Potential Energy

机译:气候变化下的风暴赛道:利用曲金的均值潜在能量实现机械理解

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摘要

Zonal-mean storm-track shifts in response to perturbations in climate occur even in idealized simulations of dry atmospheres with axisymmetric forcing. Nonetheless, a generally accepted theory of the mechanisms controlling the storm-track shifts is still lacking. Here, mean available potential energy (MAPE), a general measure of baroclinicity that is proportional to the square of the Eady growth rate, is used to understand storm-track shifts. It is demonstrated that, in dry atmospheres, the eddy kinetic energy (EKE) in a storm track is linearly related to the mean available potential energy, relative to a local reference state, and that maxima of the two are generally collocated in latitude. Changes in MAPE with climate are then decomposed into components. It is shown that in simulations of dry atmospheres, changes in the latitude of maximum MAPE are dominated by changes in near-surface meridional temperature gradients. By contrast, changes in the magnitude of MAPE are primarily determined by changes in static stability and in the depth of the troposphere. Atheory of storm-track shifts may build upon these findings and primarily needs to explain changes in near-surface meridional temperature gradients. The terminus of the Hadley circulation often shifts in tandem with storm tracks and is hypothesized to play an important role in triggering the storm-track shifts seen in this idealized dry context, especially in simulations where increases only in the convective static stability in the deep tropics suffice to shift storm tracks poleward.
机译:即使在具有轴对称强制性的干燥环境的理想模拟中,响应于气候扰动的划分的风暴轨道差异也是如此。尽管如此,仍然缺乏控制风暴轨道偏移的机制的普遍接受的理论。这里,平均可用的潜在能量(MAPE),与常见的生长速率平方成正比的一般性测量,用于了解风暴轨道偏移。据证明,在干燥气氛中,风暴轨道中的涡流能量(EKE)与相对于局部参考状态的平均可用势能线性相关,并且两者的最大值通常在纬度下并置于纬度中。然后将气候变化与气候分解成组件。结果表明,在干燥的环境中的模拟中,最大MAPE的纬度的变化主要由近表面优势温度梯度的变化主导。相比之下,MAPE幅度的变化主要由静态稳定性和对流层深度的变化决定。风暴轨道转变的高傲可能会在这些发现之上建立,主要需要解释近表面化的温度梯度的变化。 Hadley循环的终点通常与风暴轨道的串联转变,并假设在触发这种理想化的干燥环境中看到的风暴轨道移位时发挥重要作用,特别是在深热带深入对流静态稳定性上增加的模拟中足以改变风暴轨道轨道。

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