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Asymmetric thermodynamic structure of monsoon depression revealed inmicrowave satellite data

机译:季风低压的不对称热力学结构揭示了微波卫星数据

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The central parts of India receive 80-90 percent of rainfall during the monsoon season (June-September). A major portion of rainfall occurring over these parts is associated with monsoon depressions moving across the area. During the monsoon season, generally 6-7 monsoon depressions form over north Bay of Bengal and move along the monsoon trough. These systems have the potential to produce widespread distribution, with very heavy to exceptionally heavy rainfall. These synoptic systems attracted the attention for serious research by many researchers. One of the important aspects of monsoon depression is the asymmetric distribution of rainfall around its centre. Chowdhury and Gaikwad, Venkataraman et al., and Rajamani and Raoa have shown that a primary zone of the heaviest rainfall occurs in the south-west sector about 200 to 400 km from the centre, while a secondary zone of comparatively less rainfall is located about 800 km west of the depression centre. The area around the first 100 km of the depression centre is generally free from intense rainfall activities. Rajamani and Rao suggested that this observed feature of maximum zone of rainfall over the south-west sector can be explained by the omega (to) equation for the vertical velocity. Due to the maximum pressure gradient south of the centre, the maximum vorticity at the surface would be in that region and minimum at west to north-west. Rao speculated that at the initial stage as a depression over the sea, it might have a uniform pattern of rainfall. Due to paucity of observations over the north Bay of Bengal, this aspect was however not confirmed. The distribution of water vapour, cloud amount, and cloud liquid water content around the depression over the sea are also not examined. With the availability of geophysical products derived from microwave satellite data, it is now possible to examine these aspects more in detail. Two main objectives of this scientific communication are: (i) To demonstrate the potential of use of satellite microwave radiometry, for monitoring the formation and development of synoptic systems like monsoon depression over the sea. (ii) To confirm the asymmetric thermodynamic structure of monsoon depression during the initial stage of depression over the sea, where it is stationary.
机译:印度中部地区在季风季节(6月至9月)接受80%至90%的降雨。这些地区大部分降雨与季风洼地横穿整个地区有关。在季风季节,孟加拉北部湾上通常形成6-7个季风凹陷,并沿着季风槽移动。这些系统有可能产生广泛的分布,降雨非常大到异常大。这些天气系统引起了许多研究人员的重视,引起了人们的重视。季风低压的重要方面之一是其中心周围降雨的不对称分布。 Chowdhury和Gaikwad,Venkataraman等人以及Rajamani和Raoa表明,降雨量最大的主要区域发生在距中心约200至400 km的西南地区,而次区域的降雨量相对较少抑郁中心以西800公里。抑郁中心的前100公里周围通常没有强降雨活动。拉贾马尼(Rajamani)和拉奥(Rao)认为,这种观测到的西南地区最大降雨区的特征可以用垂直速度的欧米伽(to)方程解释。由于中心以南的最大压力梯度,地表的最大涡度将在该区域,而从西到西北则最小。 Rao推测,在最初阶段,由于海洋上的洼地,可能会有统一的降雨模式。由于对孟加拉北部海湾的观测稀少,这一方面尚未得到证实。还没有研究海底凹陷周围水蒸气的分布,云量和云液态水含量。随着微波卫星数据衍生的地球物理产品的可用性,现在有可能更详细地研究这些方面。这种科学交流的两个主要目标是:(i)展示使用卫星微波辐射测量技术的潜力,以监测天气系统的形成和发展,如海洋季风低压。 (ii)确认季风低压在不动的海上低压初始阶段的不对称热力学结构。

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