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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Vertical distribution of the different types of aerosols in the stratosphere: Detection of solid particles and analysis of their spatial variability
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Vertical distribution of the different types of aerosols in the stratosphere: Detection of solid particles and analysis of their spatial variability

机译:平流层中不同类型气溶胶的垂直分布:固体颗粒的检测及其空间变异性分析

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摘要

Stratospheric aerosols play a significant role in stratospheric chemistry. In the past, it was assumed that only liquid droplets are present in the stratosphere. Nevertheless, a few lidar measurements have shown that sudden enhancement of aerosol content in the middle stratosphere could be due to meteoritic debris. Aircraft measurements have shown that solid particles can be found in the lower stratosphere; these particles are mainly soot, but also include some interplanetary material. In order to better document the various characteristics of aerosols in the unperturbed stratosphere (i.e., free of volcanic aerosols), we have performed observations using different balloon-borne instruments (Stratospheric and Tropospheric Aerosol Counter (STAC), Spectroscopie d'Absorption Lunaire pour l'Observation des Minoritaires Ozone et NOx (SALOMON), and Micro Radiomètre Ballon (MicroRADIBAL)) and also some satellite data (Global ozone monitoring by occultation of stars Envisat (GOMOS-Envisat)). These instruments allow us to obtain the number of particles in different size classes, the wavelength dependence of aerosol extinction, and the radiance of the light scattered by aerosols. Combining all the data together, it appears that significant amounts of particles are ubiquitous in the middle stratosphere, above the canonical sulfate aerosol layer. “Background” interplanetary dusts in low concentration are likely present in the stratosphere. Above 30 km, interplanetary dust and largest grains from meteoroid disintegration dominate. Although the disintegration of meteoroids occurs in the upper stratosphere or in the mesosphere at all latitudes, these solid aerosols can be transported to the polar regions by the general circulation and can descend into the middle and lower stratosphere during winter mesospheric descents. Between about 22 km and 30 km, soot particles contribute to the population of aerosols at all latitudes. These soot, likely originating from biomass burning at all latitudes, could be injected into the lower stratosphere by the pyroconvective effect and can then reach the middle stratosphere perhaps owing to the gravitophotophoresis effect as was theoretically proposed. In the lower unperturbed stratosphere, liquid sulfate aerosols dominate, although soot particles are still present. Local horizontal and vertical enhancements of solid aerosols have sometimes been detected, although their origin is not yet determined. The presence of these solid particles can strongly bias the interpretation of in situ and remote sensing measurements when only the presence of liquid aerosols is assumed. Therefore, a new strategy of measurement will be necessary in the future to better characterize the stratospheric aerosol content free of volcanic particles.
机译:平流层气溶胶在平流层化学中起着重要作用。在过去,假设平流层中仅存在液滴。然而,一些激光雷达测量结果表明,平流层中层气溶胶含量突然增加可能是由于陨石碎片造成的。飞机测量结果表明,在平流层下部可以发现固体颗粒。这些颗粒主要是煤烟,但也包括一些行星际材料。为了更好地记录未受扰动的平流层中气溶胶的各种特征(即不含火山气溶胶),我们使用了不同的气球传播仪器(平流层和对流层气溶胶计数器(STAC),光谱吸收法)进行了观测。 《微量臭氧和氮氧化物的观测》(SALOMON),以及微型放射计气球(MicroRADIBAL),还有一些卫星数据(通过对卫星进行Envisat掩星进行全球臭氧监测(GOMOS-Envisat))。这些仪器使我们能够获得不同尺寸类别的颗粒数量,气溶胶消光的波长依赖性以及气溶胶散射光的辐射度。将所有数据组合在一起,似乎在标准硫酸盐气溶胶层上方的平流层中部存在大量颗粒。平流层中可能存在低浓度的“背景”行星际尘埃。在30 km以上,行星际尘埃和流星体崩解产生的最大颗粒占主导地位。尽管流星体的分解发生在所有纬度的平流层上部或中层,但这些固体气溶胶可以通过普遍循环运到极地,并在冬季中层下降时下降到平流层中下部。在大约22 km至30 km之间,烟尘颗粒会在所有纬度上导致气溶胶的数量增加。这些烟灰可能来自所有纬度的生物质燃烧,可以通过热对流作用注入平流层下部,然后可能由于理论上的重力光电泳效应而到达平流层中部。在平流层较低的下部,尽管仍然存在烟灰颗粒,但液态硫酸盐气溶胶占主导地位。尽管尚未确定固体气溶胶的水平和垂直局部增强作用,但有时尚未确定。当仅假设存在液体气溶胶时,这些固体颗粒的存在会严重影响原位和遥感测量的解释。因此,将来有必要采用一种新的测量策略,以更好地表征无火山颗粒的平流层气溶胶含量。

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