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North African mineral dust sources: new insights from a combined analysis based on 3D dust aerosol distributions, surface winds and ancillary soil parameters

机译:北非矿物粉尘来源:基于3D粉尘气溶胶分布,表面风和辅助土壤参数的组合分析新见解

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Mineral dust aerosol is a key player in the climate system. Determining dust sources and the spatio-temporal variability of dust emission fluxes is essential for estimating the impact of dust on the atmospheric radiation budget, cloud and precipitation formation processes, the bio-productivity and, ultimately, the carbon cycle. Although much effort has been put into determining dust sources from satellite observations, geo-locating active dust sources is still challenging and uncertainties in space and time are evident. One major source of uncertainty is the lack of clear differentiation between near-source dust aerosol and transported dust aerosol. In order to reduce this uncertainty, we use 3D information on the distribution of dust aerosol suspended in the atmosphere calculated from spectral measurements obtained by the Infrared Atmospheric Sounding Interferometer (IASI) by using the Mineral Aerosols Profiling from Infrared Radiance (MAPIR) algorithm. In addition to standard dust products from satellite observations, which provide 2D information on the horizontal distribution of dust, MAPIR allows for the retrieval of additional information on the vertical distribution of dust plumes. This ultimately enables us to separate between near-source and transported dust plumes. Combined with information on near-surface wind speed and surface properties, low-altitude dust plumes can be assigned to dust emission events and low-altitude transport regimes can be excluded. Consequently, this technique will reduce the uncertainty in automatically geo-locating active dust sources. The findings of our study illustrate the spatio-temporal distribution of North African dust sources based on 9 years of data, allowing for the observation of a full seasonal cycle of dust emissions, differentiating morning and afternoon/evening emissions and providing a first glance at long-term changes. In addition, we compare the results of this new method to the results from Schepanski et al. (2012), who manually identified dust sources from Spinning Enhanced Visible and InfraRed Imager (SEVIRI) red–green–blue (RGB) images. The comparison illustrates that each method has its strengths and weaknesses that must be taken into account when using the results. This study is of particular importance for understanding future environmental changes due to a changing climate.
机译:矿物粉尘气溶胶是气候系统中的关键球员。确定灰尘源和灰尘排放助熔剂的时空变异对于估算灰尘对大气辐射预算,云和降水形成过程,生物生产率以及最终碳循环的影响至关重要。虽然已经努力确定了从卫星观察结果中确定灰尘来源,但地理位置的有效灰尘来源仍然是挑战性,并且空间和时间的不确定性是显而易见的。一个主要的不确定性来源是近源尘埃气溶胶和运输尘埃气溶胶之间的明显差异。为了减少这种不确定性,我们使用3D信息通过使用从红外线辐射(MAPIR)算法的矿泉溶解率通过红外大气探测干涉干涉干涉干涉干涉干涉干涉干涉干涉干涉干涉干涉干涉干涉干涉仪(IASI)悬浮在大气中悬浮的大气中的灰尘气溶胶的分布。除了从卫星观察的标准粉尘产品外,提供有关灰尘水平分布的2D信息,MAPIR允许检索有关灰尘垂直分布的附加信息。这最终使我们能够分离近源和运输的尘埃羽毛。结合有关近表面风速和表面特性的信息,可以将低空粉尘羽线分配给灰尘发射事件,并且可以排除低空传输制度。因此,该技术将减少自动地理定位有源灰尘源的不确定性。我们的研究结果表明了基于9年的数据的北非尘埃来源的时空分布,允许观察尘埃排放的全季节性循环,区分早间和下午/晚的排放,并在长期以来一目了然-term更改。此外,我们将此新方法的结果与Schepanski等人的结果进行比较。 (2012),他手动识别来自纺纱增强的可见和红外成像器(Seviri)红绿蓝(RGB)图像的灰尘来源。比较说明了每种方法都有其强度和弱点,必须在使用结果时考虑。由于气候变化,这项研究特别重要了解未来的环境变化。

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