2022
DOI: 10.31223/x5qd36
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A review of coarse mineral dust in the Earth system

Abstract: Mineral dust particles suspended in the atmosphere span more than three orders of magnitude in diameter, from less than 0.1 µm to more than 100 µm. This wide size range makes dust a unique aerosol species with the ability to interact with many aspects of the Earth system, including radiation, clouds, hydrology, atmospheric chemistry, and biogeochemistry. This review focuses on coarse and super-coarse dust aerosols, which we respectively define as dust particles with a diameter between 2.5 - 10 µm and 10 - 62.5… Show more

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Cited by 5 publications
(23 citation statements)
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“…Absorption increases more strongly with particle size than scattering, and so the single-scattering albedo (SSA, the ratio of scattered radiation to total extinguished radiation) decreases with particle size. Indeed, submicron dust has an SSA close to 1, whereas supermicron dust absorbs a substantial fraction of the extinguished radiation, exhibiting SSAs of ~0.95 at D = 2 μm, ~0.80 at D = 10 μm and even lower for super-coarse dust 29,33 .…”
Section: Interactions With Radiationmentioning
confidence: 99%
“…Absorption increases more strongly with particle size than scattering, and so the single-scattering albedo (SSA, the ratio of scattered radiation to total extinguished radiation) decreases with particle size. Indeed, submicron dust has an SSA close to 1, whereas supermicron dust absorbs a substantial fraction of the extinguished radiation, exhibiting SSAs of ~0.95 at D = 2 μm, ~0.80 at D = 10 μm and even lower for super-coarse dust 29,33 .…”
Section: Interactions With Radiationmentioning
confidence: 99%
“…Because absorption increases more strongly with particle size than scattering 34,35 , the singlescattering albedo (SSA; the ratio of scattered radiation to total extinguished radiation) decreases with particle size. Indeed, submicron dust has an SSA close to 1, whereas supermicron dust absorbs a substantial fraction of extinguished radiation, exhibiting SSAs of ~0.95 at D = 2 µm, ~0.80 at D = 10 µm, and even lower for super coarse dust 30,36 .…”
Section: Interactions With Radiationmentioning
confidence: 99%
“…3) 6,32,46,[49][50][51][52] ; these estimates use realistic optical properties 45 and size distributions that are consistent with satellite constraints on the LW direct radiative effect 48,57 . The range reflects uncertainties in dust LW optical properties 45 , the height of dust plumes 58,59 , the dust size distribution and the contribution of super coarse dust 36,49,54 , and the effect of LW scattering by dust, which is neglected in climate models 32,33 and is sometimes accounted for using a simple correction factor 6,32,46,52 .…”
Section: Interactions With Radiationmentioning
confidence: 99%
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