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首页> 外文期刊>Annales Geophysicae >Dust aerosols over India and adjacent continents retrieved using METEOSAT infrared radiance brPart I: sources and regional distribution
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Dust aerosols over India and adjacent continents retrieved using METEOSAT infrared radiance brPart I: sources and regional distribution

机译:利用METEOSAT红外辐射在印度及邻近大陆上回收的粉尘气溶胶第一部分:来源和区域分布

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Mineral dust constitutes the single largest contributorto continental aerosols. To accurately assess the impact of dust aerosols onclimate, the spatial and temporal distribution of dust radiative propertiesis essential. Regional characteristics of dust radiative properties,however, are poorly understood. The magnitude and even sign of dustradiative forcing is uncertain, as it depends on a number of parameters, suchas vertical distribution of dust, cloud cover and albedo of the underlyingsurface. In this paper, infrared radiance (10.5-12.5 µm), acquired fromthe METEOSAT-5 satellite ( resolution), was used to retrieve regionalcharacteristics of dust aerosols for all of 1999. The infrared radiancedepression, due to the presence of dust in the atmosphere, has beenused as an index of dust load, known as the Infrared Difference Dust Index(IDDI). There have been several studies in the past carried out over the Saharausing IDDI as a measure of dust load. Over the Indian region, however,studies on dust aerosols are sparse. Spatial and temporal variability indust loading and its regional distribution over various arid and semiaridregions of India and adjacent continents (0-35° N;30° E-100° E)(excluding Sahara) have been studied and the results are examined along withsurface soil conditions (such as vegetation cover and soil moisture).The advantage of the IDDI method is that information on aerosol properties, such aschemical composition or microphysical properties, is not needed. A largeday-to-day variation in IDDI was observed over the entire study region, withvalues ranging from 4 to 22 K. It was observed that dust activity starts byMarch over the Indian deserts, as well as over deserts of the Africa and Arabianregions. The IDDI reaches maximum during the period of May to August. Regionalmaps of IDDI, in conjunction with biomass burning episodes(using TERRA satellite fire pixel counts), suggest that large IDDI valuesobserved during the winter months over Northern India could be due to a possibledeposition of black carbon on larger dust aerosols. The IDDI values havebeen compared with another year (i.e. 2003), with a large number of duststorms reported by meteorological departments based on visibility data.During the dry season, the magnitude of the monthly average IDDI during 2003 wasslightly higher than that of 1999. The monthly mean IDDI was in the range from 4to 9 K over the Indian deserts, as well as over the deserts of Africa and Arabia. Themaximum IDDI during a month was in the range from 6 to 18 K.Large IDDI values were observed even over vegetated regions (such asthe vegetated part of Africa and central India), attributed to the presence oftransported dust from nearby deserts.
机译:矿物粉尘是造成大陆气溶胶的最大因素。为了准确评估粉尘气溶胶对气候的影响,粉尘辐射特性的时空分布至关重要。然而,人们对灰尘辐射特性的区域特征了解甚少。尘埃辐射强迫的大小甚至迹象是不确定的,因为它取决于许多参数,例如尘埃的垂直分布,云量和下垫面的反照率。本文使用从METEOSAT-5卫星(分辨率)获得的红外辐射(10.5-12.5 µm)来检索1999年全年的粉尘气溶胶区域特征。由于大气中存在灰尘,红外辐射降低,已被用作粉尘负荷指数,称为红外差粉尘指数(IDDI)。过去在Saharausing IDDI上进行过数项研究,以作为粉尘负荷的量度。然而,在印度地区,关于粉尘气溶胶的研究很少。研究了印度和邻近大陆(0-35°N; 30°E-100°E)(不包括撒哈拉)的各个干旱和半干旱地区的粉尘载荷及其时空分布及其区域分布,并与表层土壤一起研究了结果IDDI方法的优点是不需要有关气溶胶特性的信息,例如化学成分或微物理特性。在整个研究区域内,IDDI每天都有很大的变化,其值在4至22 K之间。观察到,尘埃活动始于3月,开始于印度沙漠以及非洲和阿拉伯区域的沙漠。 IDDI在5月到8月期间达到最大值。 IDDI的区域地图,结合生物质燃烧事件(使用TERRA卫星火象素计数),表明印度北部冬季冬季观察到的IDDI值较大,可能是由于较大的粉尘气溶胶可能沉积了黑碳。与另一年(即2003年)相比,IDDI值已经发生了变化,当时气象部门根据能见度数据报告了许多沙尘暴。在旱季,2003年期间IDDI的月平均水平略高于1999年。印度沙漠以及非洲和阿拉伯沙漠的月平均IDDI在4至9 K的范围内。一个月内的最大IDDI在6至18 K范围内。即使在植被覆盖的地区(例如非洲和印度中部的植被覆盖地区),也观察到较大的IDDI值,这归因于附近沙漠中传播的灰尘。

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