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首页> 外文期刊>ournal of the Meteorological Society of Japan >Lidar Observation and Numerical Simulation of a Kosa (Asian Dust) over Tsukuba, Japan during the Spring of 1986
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Lidar Observation and Numerical Simulation of a Kosa (Asian Dust) over Tsukuba, Japan during the Spring of 1986

机译:1986年春季在日本筑波市上空的一种亚洲尘埃的激光雷达观测和数值模拟

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A number of duststorms and/or sandstorms occurred in the deserts and loesslands of the Asian Continent in early March of 1986. After a few days the dust laden air was transported over the Yellow Sea to Japan by westerly winds. On 12-13 March, a number of Japanese meteorological observatories reported a "Kosa (Asian dust)"phenomenon. The lidar observation of the Kosa was made at Tsukuba, Japan from 15 JST to 21 JST on 13 March 1986. The vertical structure and time change of the Kosa layer observed by the lidar are presented.At 15 JST, two Kosa layers existed at 4km and 2km, respectively. The upper layer had a thickness of about 1km and a scattering ratio of 3.2. The lower layer had a scattering ratio of 2.6 and appeared to be mixed with background aerosols. Subsequently, the Kosa layer at 4km increased in thickness and scattering intensity, with a thickness of 1.5km and a scattering ratio of 5.7. At 18 JST the Kosa layer at 4km separated into two sublayers at 4.5km and 3.5km. The total thickness of the upper and lower sublayers was 2.3km. The lidar derived optical thickness was 0.086 (wavelength 694.3nm). From 18 to 20 JST, the Kosa layer gradually lowered 0.5km. At 20 JST the Kosa layer separated into three sublayers at 4.0km, 3.2km and 2.7km. Analysis of concurrent radiosonde data showed that the upper and lower sublayers were dry, while the middle sublayer was humid.A numerical simulation was carried out to investigate the long range transport of the Kosa particles. Simulated horizontal and vertical distributions of the tracers were in good agreement with the lidar observation at Tsukuba and the routine meteorological observations in Japan and China. In particular, the observed structure of the two Kosa layers was well simulated. The two Kosa layers were found to originate from different altitudes over the source regions. The numerical simulation reveals the Loess Plateau and its neighboring deserts as important sources for the Kosa. Another possibility includes the Takla Makan Desert. Travel time of the Kosa particles to reach Japan was two to three days from the Loess Plateau and its neighboring deserts, and five to six days from the Takla Makan Desert.
机译:1986年3月上旬,在亚洲大陆的沙漠和黄土地区发生了许多沙尘暴和/或沙尘暴。几天后,载有尘埃的空气被西风吹过黄海,运往日本。 3月12日至13日,日本许多气象台报道了“亚洲尘埃”现象。 Kosa的激光雷达观测是在1986年3月13日在日本筑波的15 JST到21 JST进行的。呈现了由激光雷达观测的Kosa层的垂直结构和时间变化。在15 JST时,在4 km处存在两个Kosa层和2公里。上层的厚度约为1km,散射比为3.2。下层的散射比为2.6,似乎与背景气溶胶混合。随后,4公里处的Kosa层的厚度和散射强度增加,厚度为1.5公里,散射比为5.7。在日本标准时间18日,4公里处的Kosa层在4.5公里和3.5公里处分成两个子层。上下子层的总厚度为2.3公里。激光雷达得出的光学厚度为0.086(波长694.3nm)。从日本标准时间18到20,科萨层逐渐降低了0.5公里。在20 JST时,Kosa层在4.0km,3.2km和2.7km处分成三个子层。同时进行的探空仪数据分析表明,上,下子层是干燥的,而中子层是潮湿的。通过数值模拟研究了Kosa粒子的远距离传输。示踪剂的模拟水平和垂直分布与筑波的激光雷达观测以及日本和中国的常规气象观测非常吻合。特别是,很好地模拟了两个Kosa层的观察结构。发现这两个科萨层起源于源区的不同高度。数值模拟表明,黄土高原及其附近的沙漠是科萨的重要来源。另一个可能性包括塔克拉马卡沙漠。从黄土高原及其邻近的沙漠到科萨颗粒到达日本的时间为两到三天,而从塔克拉玛坎沙漠出发则为五到六天。

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