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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Characteristics and origin of quasi-biweekly oscillation over the western North Pacific during boreal summer
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Characteristics and origin of quasi-biweekly oscillation over the western North Pacific during boreal summer

机译:北方夏季北部太平洋西部准双周振荡的特征和成因

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摘要

This study investigates the structure, energetic, and origin of quasi-biweekly oscillation (QBWO) over the western North Pacific (WNP), using NCEP reanalyses for the years 2000-2007. In the context of vorticity there appears to be a significant QBWO mode over the WNP during the summer. QBWO emerges from the equatorial region and propagates northwestward. Its horizontal structure exhibits a slight southwest-northeast tilt but mainly longitudinal elongation. In the vertical the QBWO has a northwest tilt with height that gives rise to a structure of the first baroclinic mode. The centers of vorticity and vertical motion near the equator show a phase lag of about one-quarter wavelength, consistent with the characteristics of equatorial waves, whereas the cyclonic circulation is tightly coupled with anomalous convection as the wave moves away from the equator. Energetic analysis of the QBWO reveals that diabatic heating in the tropics and baroclinic processes in the subtropics play important roles in the generation of eddy available potential energy (EAPE). In turn, the conversion from EAPE to eddy kinetic energy (EKE) and the barotropic conversion are major sources for EKE to compensate the loss by EKE redistribution and dissipation. Tracing the QBWO to equatorial disturbances, our results show some features of equatorially trapped n = 1 Rossby mode, such as phase speed and group velocity. This mode is generally characterized by a zonal planetary wave number of about 6 and nearly symmetric circulation about the equator. A typical case from 2002 is chosen to illustrate that the origin of the QBWO is closely associated with the theoretical equatorial Rossby wave.
机译:这项研究使用2000-2007年的NCEP重新分析,研究了北太平洋西部(WNP)上的准双周振荡(QBWO)的结构,能量和成因。在涡旋的背景下,夏季似乎在WNP上存在明显的QBWO模式。 QBWO从赤道地区出现并向西北传播。它的水平结构表现出轻微的西南-东北倾斜,但主要是纵向伸长。在垂直方向上,QBWO具有向西北倾斜的高度,从而产生了第一斜斜模式的结构。赤道附近的涡旋和垂直运动中心显示出大约四分之一波长的相位滞后,与赤道波的特征一致,而旋风环流与异常对流紧密地耦合在一起,因为该波远离赤道。对QBWO的能量分析表明,热带的非绝热加热和亚热带的斜压过程在产生涡流可用势能(EAPE)中起着重要作用。反过来,从EAPE到涡动能(EKE)的转换以及正压转换是EKE通过EKE重新分配和耗散补偿损失的主要来源。追踪QBWO到赤道扰动,我们的结果显示了赤道被困n = 1 Rossby模式的一些特征,例如相速度和群速度。该模式的特征通常是约6的纬向行星波数和围绕赤道的近似对称环流。选择2002年的一个典型案例来说明QBWO的起源与理论赤道Rossby波密切相关。

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