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The radiative impact of airborne dust on the Saharan cyclone on February 2007.

机译:2007年2月在撒哈拉旋风上的空气灰尘对撒哈拉飓风的辐射影响。

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The dust activity over North Africa associated with the Saharan depression event in February 2007 is investigated by mean of spaceborne observations and ground based measurements. The main characteristics of the cyclone as well as the meteorological conditions during this event are described using the European Centre for Medium-range Weather Forecasts (ECMWF). The dust storm and cloud cover over North Africa is thoroughly described combining for the first time Spinning Enhanced Visible and Infra-Red Imager (SEVIRI) images for the spatio-temporal evolution and Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) and CloudSat observations for the vertical distribution. The Saharan depression formed over Algeria in the lee of the Atlas Mountain on the afternoon of February 20 in response to midlatitude trough intrusion. It migrated eastward with a speed of 11 m s~(-1) and reached Libya on February 22 before exiting the African continent toward the Mediterranean Sea on February 23. The cyclone provided a dynamical forcing that led to strong near-surface winds and produced a major dust storm over North Africa. Heavy dust load was seen along the cold front and the southeastern edge of the cyclone accompanied by a deep cloud band along its northwestern edge. The dust was transported all around the cyclone leaving a clear eye on its centre (Fig. 1). On the vertical, slanted dust layers were consistently observed during the event over North Africa. Furthermore, the dust was lofted to altitudes as high as 7 km (Fig. 1), becoming subject to long range transport. The radiative forcing of dust and its feedback on the cyclone dynamics has been evaluated using a mesoscale model. The comparison between the simulations with and without dust has suggested that the radiative impact of dust represents important implications on the dynamics and the lifetime of the cyclone. A local heating of 3 K at 1 km was induced by the presence of the airborne dust in the atmosphere.
机译:通过星源观测和基于地面测量的平均值来研究与撒哈拉抑郁症活动相关的北非粉尘活动。使用欧洲的中距离天气预报(ECMWF)描述了旋风内的主要特征以及该事件期间的气象条件。北非的尘埃风暴和云覆盖是彻底描述的第一次旋转增强的可见和红外图像(Seviri)图像,用于时空进化和云 - 气溶胶激光葡萄球和红外探测器卫星观察(Calipso)和Cloudsat垂直分布的观察。 2月20日的下午,在阿尔及利亚在阿尔及利亚形成了阿尔及利亚,于2月20日的下午响应了中间槽侵入。它以东10号速度向东迁移到11毫秒〜(1),并于2月22日达到利比亚,然后于2月23日离开非洲大陆。旋风提供了一种动态强迫,导致了强大的近地风和产生了北非的主要尘暴风暴。沿着旋风沿着沿着西北边缘的深云带,沿着旋风的圆形边缘看到大粉尘负荷。灰尘在旋风分离器周围运输,留在其中心上的透明眼睛(图1)。在北非在北非事件期间始终观察到垂直的粉尘层。此外,灰尘使灰尘高达7 km(图1),变得越来越长。使用MESCLE模型评估了粉尘的辐射强制及其对旋风动力学的反馈。模拟与无灰尘之间的比较表明灰尘的辐射影响是对动态和旋风器的寿命的重要意义。通过在大气中的空气灰尘存在,诱导3 k局部加热3 k。

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