We have developed techniques to map the distribution and composition of cla
y-rich soils with portable field spectrometers on the ground. Spectral refl
ectance measurements in the 1800-2400-nm region with 10-nm resolution can d
istinguish smectites, which cause swelling, from illites and kaolinite that
do not swell significantly. Illites and smectites are often mixed in the s
oil and result in varying swell potential. Standard engineering soil tests
are too time consuming and costly to be used in areas where there is highly
varying swell potential. Therefore, in many instances in regions of steepl
y dipping sedimentary layers, beds of swelling clay go undetected. We show
that it is possible to determine smectite content with a standard cross-val
idation error of 10% based on partial least-squares analysis of second-deri
vative reflectance spectra. Loadings show that the 1800-2000- and 2150-2250
-nm regions contain the most relevant information for the detection and qua
ntification of smectite content and these correspond to the bound water in
the clay lattice interlayer and the Al-OH combination band, respectively. C
orrelations as high as 87% were obtained with the Seed swell-potential inde
x. The correlations are higher when the samples were dried rather than meas
ured in their moist condition shortly after collection in the field, as in
an earlier study. Correlation with other swell indices shows that reflectan
ce spectroscopy would be a reliable indicator that could divide samples int
o low, medium, and high swell potential. The effect of sample moisture was
studied and the results show that the surface of the field samples must fir
st be dried before measurement, in order to obtain a reliable swell potenti
al value from the model. (C) 2001 John Wiley & Sons, Inc.