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Optical, microphysical and compositional properties of the Eyjafjallaj?kull volcanic ash

机译:眼影jallaj的光学,微物理和组成特性?kull火山灰

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Better characterization of the optical properties of aerosol particles are an essential step to improve atmospheric models and satellite remote sensing, reduce uncertainties in predicting particulate transport, and estimate aerosol forcing and climate change. Even natural aerosols such as mineral dust or particles from volcanic eruptions require better characterization in order to define the background conditions from which anthropogenic perturbations emerge. We present a detailed laboratorial study where the spectral optical properties of the ash from the April–May (2010) Eyjafjallaj?kull volcanic eruption were derived over a broad spectral range, from ultra-violet (UV) to near-infrared (NIR) wavelengths. Samples of the volcanic ash taken on the ground in the vicinity of the volcano were sieved, re-suspended, and collected on filters to separate particle sizes into fine and mixed (coarse and fine) modes. We derived the spectral mass absorption efficiency abs [m2g1] for fine and mixed modes particles in the wavelength range from 300 to 2500 nm from measurements of optical reflectance. We retrieved the imaginary part of the complex refractive index Im(m) from abs, using Mie–Lorenz and T-matrix theories and considering the size distribution of particles obtained by scanning electron microscopy (SEM), and the grain density of the volcanic ash measured as = 2.16 ± 0.13 g cm3. Im(m) was found to vary from 0.001 to 0.005 in the measured wavelength range. The dependence of the retrieval on the shape considered for the particles were found to be small and within the uncertainties estimated in our calculation. Fine and mixed modes were also analyzed by X-ray fluorescence, exhibiting distinct elemental composition supporting the optical differences we found between the modes. This is a comprehensive and consistent characterization of spectral absorption and imaginary refractive index, density, size, shape and elemental composition of volcanic ash, which will help constrain assumptions of ash particles in models and remote sensing, thereby narrowing uncertainties in representing these particles both for short-term regional forecasts and long-term climate change.
机译:更好地表征气溶胶颗粒的光学性质是改善大气模型和卫星遥感的基本步骤,减少预测颗粒式运输的不确定性,并估算气溶胶迫使和气候变化。即使是来自火山爆发的矿物粉尘或颗粒的天然气溶胶也需要更好的表征,以便定义从中扰动的背景条件出现。我们介绍了一个详细的实验室研究,其中Ash从4月 - 5月(2010)eyjafjallaj?kull火山喷发的灰分的光谱光学性质衍生在广谱范围内,从紫外(UV)到近红外(NIR)波长。在火山附近的地面上拍摄的火山灰样品被筛分,重新悬挂,并在过滤器上收集以将粒度分离成细小和混合(粗细胞)模式。我们在波长范围内的微量和混合模式颗粒的光谱质量吸收效率ABS [M2G1]从光学反射测量的测量范围内的微量和混合模式。通过使用Mie-Lorenz和T基质理论,并考虑通过扫描电子显微镜(SEM)获得的粒子的尺寸分布,以及通过扫描电子显微镜(SEM)和火山灰的晶粒密度来检索来自ABS的虚拟折射率IM(M)的虚部分布测量为= 2.16±0.13g cm3。发现IM(m)在测量的波长范围内从0.001至0.005变化。检索对所考虑的颗粒的形状的依赖性被发现小并且在我们计算中估计的不确定性内。还通过X射线荧光分析精细和混合模式,表现出支持在模式之间发现的光学差异的不同元素组合物。这是火山灰的光谱吸收和假想折射率,密度,尺寸,形状和元素组成的全面且一致的表征,这将有助于限制灰分粒子在模型和遥感中的假设,从而缩小代表这些颗粒的不确定性短期区域预测和长期气候变化。

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