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Mesoscale Convective Vortices Observed during BAMEX. Part Ⅱ: Influences on Secondary Deep Convection

机译:在BAMEX期间观测到的中尺度对流涡旋。第二部分:对二次深对流的影响

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Observations from the Bow Echo and Mesoscale Convective Vortex (MCV) Experiment are used to examine the role of the five mesoscale convective vortices described in Part Ⅰ on heavy precipitation during the daytime heating cycle. Persistent widespread stratiform rain without deep convection occurs for two strong MCVs in conditionally stable environments with strong vertical shear. Two other MCVs in moderate-to-strong vertical shear have localized redevelopment of deep convection (termed secondary convection) on their downshear side, where conditional instability exists. The strongest of the five MGVs occurs in weak vertical shear and has widespread secondary convection, which is most intense on its conditionally unstable southeast periphery. The two MCVs with only localized secondary convection have well-defined mesoscale vertical motion couplets with downshear ascent and upshear descent above the planetary boundary layer (PBL). Although the amplitude is significantly greater, the kinematically derived vertical motion dipole resembles that implied by steady, vortex-relative isentropic flow, consistent with previous idealized (dry) simulations and diagnoses based on operational model analyses. In the other three cases with either widespread precipitation or weak environmental vertical shear, the kinematic and isentropic vertical motion patterns are poorly correlated. Vertical motions above the PBL provide a focus for secondary convection through adiabatic cooling downshear and adiabatic warming upshear of the MCV center. The MCVs occur within surface frontal zones with large temperature and moisture gradients across the environmental vertical shear vector (Part Ⅰ). Thus, the effect of vertical motions on conditional instability is reinforced by horizontal advections of high equivalent potential temperature air downshear, and low equivalent potential temperature air upshear within the PBL. On average, the quadrant immediately right of downshear (typically southeast of the MCV center) best supports deep convection because of the juxtaposition of greatest mesoscale ascent, high equivalent potential temperature PBL air, and MCV-induced enhancement of the vertical shear.
机译:利用弓形回波和中尺度对流涡旋(MCV)实验观察了第一部分所述的五个中尺度对流涡旋在白天加热周期中对强降水的作用。在条件稳定且垂直剪切力强的环境中,两个强MCV会持续发生没有深对流的持久层状降雨。在中等至强的垂直剪切作用下的另外两个MCV在其下剪切侧存在条件不稳定的地方,发生了深对流(称为二次对流)的局部再发展。五个MGV中最强的发生在弱的垂直切变中,并具有广泛的二次对流,这在其条件不稳定的东南边缘上最为强烈。仅具有局部二次对流的两个MCV具有定义明确的中尺度垂直运动对,其中行星边界层(PBL)上方具有下降剪切上升和上升剪切下降。尽管振幅明显更大,但运动学派生的垂直运动偶极子类似于稳定的,相对于涡流的等熵流,这与以前的理想化(干式)模拟和基于运行模型分析的诊断相一致。在其他三种情况下,无论是降水量大分布还是环境垂直剪切力弱,运动学和等熵的垂直运动模式都没有很好的相关性。 PBL上方的垂直运动通过MCV中心的绝热降温剪切和绝热升温剪切为二次对流提供了焦点。 MCVs发生在整个环境垂直切向矢量上具有较大温度和湿度梯度的地表锋区中(第一部分)。因此,垂直运动对条件不稳定性的影响通过PBL内高等效电位空气下切变和低等效电位空气下切变的水平对流得到加强。平均而言,由于最大的中尺度上升,高等电位温度的PBL空气并置和MCV引起的垂直剪切力增强,下切变的右下象限(通常在MCV中心的东南方)最好地支持深度对流。

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