Dominance of goethite over hematite in iron oxides of mineral dust from Western Africa: Quantitative partitioning by X‐ray absorption spectroscopy
Open Access
- 13 October 2014
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Atmospheres
- Vol. 119 (22) , 12,740-12,754
Abstract
This paper reports on the X‐ray absorption analysis of samples of mineral dust emitted from or transported to Western Africa. We found that iron oxides account, by mass, for 38% to 72% of the total elemental iron. They are composed of minerals in the Fe(III) oxidation state: goethite (FeO·OH) and hematite (Fe2O3). The apparent fraction of iron oxide attributed to goethite is higher than hematite regardless of the source region from which the dust originated. The goethite percent content of iron oxides is in the range 52–78% (by mass), the highest values being measured for dust originating in the Sahel. The limited number of samples analyzed and the sample‐to‐sample variability prevent us from concluding firmly on the regional variability of the goethite‐to‐hematite ratio. Based on the experimental data on mineralogical composition and on concurrent measurements of the number size distribution, the optical properties of mineral dust have been calculated in a Mie approximation for homogeneous spherical particles. At 550 nm, the single‐scattering albedo ω0 ranges between 0.89 and 0.93, the asymmetry factor g ranges between 0.76 and 0.8 and the mass extinction efficiency kext varies between 0.5 and 1.1 m2 g−1; these values are all in the range of those from independent direct measurements. Neglecting the partitioning between hematite and goethite and the assimilation of iron oxides by hematite, as it is often done with models, lowers the single‐scattering albedo and increases the asymmetry factor in the UV‐visible spectral region below 550 nm. The mass extinction efficiency is insensitive to the nature of the iron oxides but rather responds to variations in the number size distribution. The mineralogy of iron oxides should therefore be taken into account when assessing the effect of mineral dust on climate and atmospheric chemistry, in particular via interactions involving photolysis.Keywords
Funding Information
- European Community's Sixth Framework Research Program
- API-AMMA French
This publication has 63 references indexed in Scilit:
- The speciation of iron in desert dust collected in Gran Canaria (Canary Islands): Combined chemical, magnetic and optical analysisAtmospheric Environment, 2008
- Mineralogy as a critical factor of dust iron solubilityGeophysical Research Letters, 2008
- Sensitivity Experiments on the Effects of Optical Properties of Dust Aerosols on Their Radiative Forcing under Clear Sky ConditionJournal of the Meteorological Society of Japan, 2005
- Radiative properties and direct effect of Saharan dust measured by the C‐130 aircraft during Saharan Dust Experiment (SHADE): 2. Terrestrial spectrumJournal of Geophysical Research: Atmospheres, 2003
- Radiative properties and direct radiative effect of Saharan dust measured by the C‐130 aircraft during SHADE: 1. Solar spectrumJournal of Geophysical Research: Atmospheres, 2003
- Combined use of satellite and surface observations to infer the imaginary part of refractive index of Saharan dustGeophysical Research Letters, 2003
- ENVIRONMENTAL CHARACTERIZATION OF GLOBAL SOURCES OF ATMOSPHERIC SOIL DUST IDENTIFIED WITH THE NIMBUS 7 TOTAL OZONE MAPPING SPECTROMETER (TOMS) ABSORBING AEROSOL PRODUCTReviews of Geophysics, 2002
- Incorporation of mineralogical composition into models of the radiative properties of mineral aerosol from UV to IR wavelengthsJournal of Geophysical Research: Atmospheres, 1999
- Aluminum-Bearing Goethite in Venezuelan LateritesClays and Clay Minerals, 1979
- Complex refractive index of limestone in the visible and infraredApplied Optics, 1978