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A Polar Low over the Japan Sea on 21 January 1997. Part Ⅱ: A Numerical Study

机译:1997年1月21日发生在日本海上的极地低压。第二部分:数值研究

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A remarkable isolated polar low observed over the Japan Sea on 21 January 1997 is studied by numerical simulations using a 20-km-mesh regional primitive equation model [Regional Spectral Model (RSM) of the Japan Meteorological Agency] and a 5-km-mesh nonhydrostatic mesoscale model [Meteorological Research Institute Nonhydrostatic Model (MRI-NHM)] and by sensitivity experiments using the MRI-NHM. The 24-h integration of RSM starting from 0000 UTC 21 January reproduces quite well the polar low's movement and development, including the initial wrapping of the west part of an east-west-oriented vorticity zone. The vorticity budget analysis indicates that the stretching term plays a dominant role in the polar low development. The simulation by MRI-NHM reproduces surprisingly well the wrapping of the western part of the east-west-oriented vortcity zone associated with a cloud band, the spiral-shaped cloud pattern, and the "eye" structure near the vortex center. The wind speed and resulting sea surface heat fluxes of the simulated polar low exhibited a significant deviation from axisymmetry. The eye, almost free of cloud, was relatively dry and was associated with a strong downdraft and a warm core. A thermodynamic budget analysis indicates that the warm core is mainly caused by the adiabatic warming due to the downdraft. Two types of sensitivity experiments using a 6-km-mesh MRI-NHM are performed: In the first type, the physical processes such as condensational heating and/or surface heat fluxes are switched on-off throughout the whole integration time of 24 h, as in the past sensitivity studies. In the second type, on the other hand, both condensational heating and surface heat fluxes are incorporated up to a certain time, but then one or all of them are switched on-off for the following 1 h. This minimizes the deformation of the environment of the vortex and is suitable for studying the direct effect of the physical processes on the vortex development. The results of the sensitivity experiments show that the rapid development of the present polar low is principally caused by the condensational heating. The surface heat fluxes, on the other hand, are important for maintaining the environment that supports the vortex development; that is, the absence of the surface heat fluxes stabilizes the stratification in the boundary layer so that the vortex development is severely suppressed.
机译:1997年1月21日在日本海上观测到的一个显着的孤立极地低压,通过使用20公里网眼的区域原始方程模型[日本气象厅的区域光谱模型(RSM)]和5公里网眼的数值模拟进行了研究。非静水中尺度模型[气象研究所非静水模型(MRI-NHM)]并通过使用MRI-NHM进行敏感性实验。从1月21日0000 UTC开始的24小时RSM整合很好地再现了极地低谷的运动和发展,包括东西向涡旋带西侧的初始包裹。涡度预算分析表明,伸展期在极地低空发育中起主导作用。 MRI-NHM进行的模拟令人惊讶地很好地再现了东西方向风蚀带的西部部分的包裹,该包裹带与云带,螺旋状云模式和涡旋中心附近的“眼”结构有关。模拟的极地低气压的风速和由此产生的海面热通量与轴对称性表现出显着偏差。眼睛几乎没有云,相对干燥,并伴有强烈的向下气流和温暖的核心。热力学预算分析表明,岩心变暖主要是由于下降气流引起的绝热变暖所致。使用6公里网孔MRI-NHM进行两种类型的灵敏度实验:在第一种类型中,在24小时的整个积分时间内,诸如冷凝加热和/或表面热通量之类的物理过程处于关闭状态,与过去的敏感性研究一样另一方面,在第二种类型中,凝结热通量和表面热通量都被合并到一定时间,但是随后一个小时或全部关闭它们中的一个或全部。这使涡旋环境的变形最小化,并且适合于研究物理过程对涡旋发展的直接影响。灵敏度实验的结果表明,当前极地低压的迅速发展主要是由凝结加热引起的。另一方面,表面热通量对于维持支持涡旋发展的环境非常重要。即,表面热通量的缺乏稳定了边界层中的分层,从而严重抑制了涡旋的发展。

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