The Open UniversitySkip to content
 

The retrieval of optical properties from terrestrial dust devil vortices

Mason, Jonathon P.; Patel, Manish P. and Lewis, Stephen (2014). The retrieval of optical properties from terrestrial dust devil vortices. Icarus, 231 pp. 385–393.

Full text available as:
Full text not publicly available (Version of Record)
Due to publisher licensing restrictions, this file is not available for public download
Click here to request a copy from the OU Author.
DOI (Digital Object Identifier) Link: https://doi.org/10.1016/j.icarus.2013.12.013
Google Scholar: Look up in Google Scholar

Abstract

The retrieval of the optical properties of desert aerosols in suspension within terrestrial dust devils is presented with possible future application for martian dust devils. The transmission of light through dust devil vortices was measured in situ to obtain the wavelength-dependent attenuation by the aerosols. A Monte Carlo model was applied to each dust devil with the retrieved optical properties corresponding to the set of parameters which lead to the best model representation of the observed transmission spectra. The retrieved optical properties agree well with single scattering theory and are consistent with previous studies of dust aerosols. The enhanced absorption observed for dust devils with a higher tangential wind speed, and in comparison to atmospheric aerosol studies, suggests that larger dust particles are lofted and suspended around dust devil vortices. This analysis has shown that the imaginary refractive indices (and thus the optical properties of the suspended dust) are generally overestimated when these larger dust grains entrained by dust devils are neglected. This will lead to an overestimation of the amount of solar radiation absorbed by the small particles that remain in suspension after the dust devil terminates. It is also demonstrated that a 10% uncertainty in the particle size distribution of the dust entrained in the dust devils can result in a 50% increase in the predicted amount of incident solar radiation absorbed by the dust particles once the dust devil has terminated. The method used here provides the capability to retrieve the optical properties of the dust entrained in martian dust devils by taking advantage of transits over surface spacecraft which are capable of making optical measurements at ultraviolet and visible wavelengths. Our results suggest that we would observed higher absorption at all wavelengths for dust particles entrained in dust devil vortices compared to the ubiquitous dust haze.

Item Type: Journal Item
Copyright Holders: 2014 Elsevier Inc.
ISSN: 0019-1035
Project Funding Details:
Funded Project NameProject IDFunding Body
Support for Science Co-I's on the ExoMars Trace Gas Orbiter InstrumentsST/I003061/1STFC (Science & Technology Facilities Council)
Light and life: Constraining the environmental conditions for life.PP/E007740/1STFC (Science & Technology Facilities Council)
NOMAD-UVIS Flight ElectronicsST/L00027X/1STFC (Science & Technology Facilities Council)
Keywords: meteorology; Earth; Mars; radiative transfer; Mars, atmosphere
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Research Group: Space
Item ID: 39641
Depositing User: Manish Patel
Date Deposited: 04 Mar 2014 16:30
Last Modified: 07 Dec 2018 20:28
URI: http://oro.open.ac.uk/id/eprint/39641
Share this page:

Metrics

Altmetrics from Altmetric

Citations from Dimensions

Actions (login may be required)

Policies | Disclaimer

© The Open University   contact the OU