Optical properties of meteoric smoke analogues

<p><strong>Abstract.</strong> Accurate determination of the optical properties of analogues for meteoric smoke particles (MSPs), which are thought to be composed of iron-rich oxides or silicates, is important for their observation and characterization in the atmosphere. In this stu...

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Main Authors: Aylett, Tasha (Author) , Brooke, James S. A. (Author) , James, Alexander D. (Author) , Nachbar, Mario (Author) , Duft, Denis (Author) , Leisner, Thomas (Author) , Plane, John M. C. (Author)
Format: Article (Journal)
Language:English
Published: 11 Oct 2019
In: Atmospheric chemistry and physics. Discussions
Year: 2019, Volume: 19, Issue: 19, Pages: 12767-12777
ISSN:1680-7375
DOI:https://doi.org/10.5194/acp-19-12767-2019
Online Access:Verlag, Volltext: https://doi.org/https://doi.org/10.5194/acp-19-12767-2019
Verlag: https://www.atmos-chem-phys.net/19/12767/2019/
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Author Notes:Tasha Aylett, James S. A. Brooke, Alexander D. James, Mario Nachbar, Denis Duft, Thomas Leisner, and John M. C. Plane

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520 |a <p><strong>Abstract.</strong> Accurate determination of the optical properties of analogues for meteoric smoke particles (MSPs), which are thought to be composed of iron-rich oxides or silicates, is important for their observation and characterization in the atmosphere. In this study, a photochemical aerosol flow system (PAFS) has been used to measure the optical extinction of iron oxide MSP analogues in the wavelength range 325-675&thinsp;nm. The particles were made photochemically and agglomerate into fractal-like particles with sizes on the order of 100&thinsp;nm. Analysis using transmission electron microscopy (TEM), energy-dispersive X-ray spectroscopy (EDX) and electron energy loss spectroscopy (EELS) suggested the particles were most likely maghemite-like (<span class="inline-formula"><i>γ</i></span>-<span class="inline-formula">Fe<sub>2</sub>O<sub>3</sub></span>) in composition, though a magnetite-like composition could not be completely ruled out. Assuming a maghemite-like composition, the optical extinction coefficients measured using the PAFS were combined with maghemite absorption coefficients measured using a complementary experimental system (the MICE-TRAPS) to derive complex refractive indices that reproduce both the measured absorption and extinction.</p> 
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