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在莫纳罗亚天文台收集的单个亚洲沙尘异质颗粒的分析与光学建模

Analysis and Optical Modeling of Individual Heterogeneous Asian Dust Particles Collected at Mauna Loa Observatory.

作者信息

Conny Joseph M, Willis Robert D, Ortiz-Montalvo Diana L

机构信息

Materials Measurement Science Division, National Institute of Standards and Technology, Gaithersburg, MD, USA.

Office of Research and Development, U.S. Environmental Protection Agency, Research Triangle Park, NC, USA (retired).

出版信息

J Geophys Res Atmos. 2019;124(5). doi: 10.1029/2018jd029387.

Abstract

We have determined optical properties of heterogeneous particles from aerosol samples collected at Hawaii's Mauna Loa Observatory. Back trajectories, satellite imagery, and composition differences among particles from scanning electron microscopy revealed a subset of particles with dolomite or calcite that likely came from Asia. Using focused ion-beam tomography and the discrete dipole approximation, we show how small amounts of an iron phase (oxide or carbonate), or in one case soot, affected extinction and scattering compared with particles of neat dolomite or calcite. We show how particles exhibit a range scattering values due to varying orientations of the inclusion phases. Extinction efficiencies for the heterogeneous particles with dolomite (3.47) and calcite (3.36) were 19% to 21% lower than extinction for marine background air particles (3.72). Extinction for the Asian dust was, however, generally higher than for the neat particles. Compared to iron carbonate, the presence of an absorbing iron oxide affected scattering in Asian dust particles even at the low oxide concentrations studied here (0.6% to 8.1%). Scattering efficiency decreased by <1% with a 1% increase in hematite but by 2% to 5% with magnetite. Asian dust scattered light strongly forward, but backscattering was 56% larger than for the marine background air particles. Backscattering in the Asian dust was also larger with magnetite than hematite. Single scattering albedo for Asian dust with hematite, magnetite, or soot averaged 0.96 ± 0.06 but was as low as 0.72 with a magnetite mass of 5.8%.

摘要

我们已经确定了从夏威夷莫纳罗亚天文台采集的气溶胶样本中异质颗粒的光学特性。反向轨迹、卫星图像以及扫描电子显微镜下颗粒之间的成分差异显示,一部分含有白云石或方解石的颗粒可能来自亚洲。通过聚焦离子束断层扫描和离散偶极近似,我们展示了与纯净白云石或方解石颗粒相比,少量铁相(氧化物或碳酸盐),或在一种情况下的烟灰,是如何影响消光和散射的。我们展示了由于包裹相取向的变化,颗粒如何呈现出一系列散射值。含有白云石(3.47)和方解石(3.36)的异质颗粒的消光效率比海洋背景空气颗粒的消光效率(3.72)低19%至21%。然而,亚洲沙尘的消光通常高于纯净颗粒。与碳酸铁相比,即使在这里研究的低氧化物浓度(0.6%至8.1%)下,吸收性氧化铁的存在也会影响亚洲沙尘颗粒的散射。赤铁矿含量每增加1%,散射效率降低不到1%,但磁铁矿会使其降低2%至5%。亚洲沙尘强烈向前散射光,但后向散射比海洋背景空气颗粒大56%。亚洲沙尘中磁铁矿的后向散射也比赤铁矿大。含有赤铁矿、磁铁矿或烟灰的亚洲沙尘的单次散射反照率平均为0.96±0.06,但当磁铁矿质量为5.8%时,单次散射反照率低至0.72。

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