Abstract. Mineral dust particles dominate aerosol mass in the atmosphere and directly
modify Earth's radiative balance through absorption and scattering. This
radiative forcing varies strongly with mineral composition, yet there is
still limited knowledge on the mineralogy of atmospheric dust. In this
study, we performed X-ray diffraction (XRD) and reflectance spectroscopy
measurements on 37 different dust deposition samples collected as airfall in
an urban setting to determine mineralogy and the relative proportions of
minerals in the dust mixture. Most commonly, XRD has been used to
characterize dust mineralogy; however, without prior special sample
preparation, this technique is less effective for identifying poorly
crystalline or amorphous phases. In addition to XRD measurements, we
performed visible and short-wave infrared (VSWIR) reflectance spectroscopy
for these natural dust samples as a complementary technique to determine
mineralogy and mineral abundances. Reflectance spectra of dust particles are
a function of a nonlinear combination of mineral abundances in the mixture.
Therefore, we used a Hapke radiative transfer model along with a linear
spectral mixing approach to derive relative mineral abundances from
reflectance spectroscopy. We compared spectrally derived abundances with
those determined semi-quantitatively from XRD. Our results demonstrate that
total clay mineral abundances from XRD are correlated with those from
reflectance spectroscopy and follow similar trends; however, XRD
underpredicts the total amount of clay for many of the samples. On the other
hand, calcite abundances are significantly underpredicted by SWIR compared
to XRD. This is caused by the weakening of absorption features associated
with the fine particle size of the samples, as well as the presence of dark
non-mineral materials (e.g., asphalt) in these samples. Another possible
explanation for abundance discrepancies between XRD and SWIR is related to
the differing sensitivity of the two techniques (crystal structure vs.
chemical bonds). Our results indicate that it is beneficial to use both XRD
and reflectance spectroscopy to characterize airfall dust because the
former technique is good at identifying and quantifying the SWIR-transparent
minerals (e.g., quartz, albite, and microcline), while the latter technique
is superior for determining abundances for clays and non-mineral components.