Articles | Volume 18, issue 13
https://doi.org/10.5194/acp-18-9681-2018
https://doi.org/10.5194/acp-18-9681-2018
Research article
 | 
10 Jul 2018
Research article |  | 10 Jul 2018

The influence of dust optical properties on the colour of simulated MSG-SEVIRI Desert Dust infrared imagery

Jamie R. Banks, Kerstin Schepanski, Bernd Heinold, Anja Hünerbein, and Helen E. Brindley

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AR: Author's response | RR: Referee report | ED: Editor decision
AR by Jamie Banks on behalf of the Authors (31 May 2018)  Author's response   Manuscript 
ED: Publish subject to minor revisions (review by editor) (11 Jun 2018) by Claire Ryder
AR by Jamie Banks on behalf of the Authors (21 Jun 2018)  Author's response   Manuscript 
ED: Publish as is (25 Jun 2018) by Claire Ryder
AR by Jamie Banks on behalf of the Authors (25 Jun 2018)
Short summary
Satellite observations are used to visualize dust storms over the Sahara, and specific infrared channel combinations can highlight dust with distinctive pink colours. Using output from a dust-atmosphere model to simulate satellite imagery, we explore the consequences of particle size, shape, and refractive index for the colour of dust in the imagery. Particles with a radius of ~ 1.5 microns perturb the colour the most and an assumption of spherical dust appears to be insufficient.
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