H. Behrens et al., NEAR-INFRARED SPECTROSCOPIC DETERMINATION OF WATER SPECIES IN GLASSESOF SYSTEM MALSI(3)O(8) (M=LI, NA, K) - AN INTERLABORATORY STUDY, Chemical geology, 128(1-4), 1996, pp. 41-63
The near-infrared absorption bands at 5200 cm(-1), assigned to molecul
ar water, and at 4500 cm(-1), assigned to hydroxyl groups bonded to ne
twork forming cations, were used to specify concentrations of water sp
ecies in glasses of alkali feldspar composition MAlSi(3)O(8) (M = Li,
Na, K). To allow an accurate quantitative evaluation of the water spec
ies in hydrous glasses, we have determined the composition dependence
of the density and the linear and integral extinction coefficients of
the glasses. For each feldspar composition, 8-28 samples with various
amounts of water have been synthesized. All samples were quenched isob
arically to avoid desorption of water during cooling, Water contents o
f the glasses were analyzed by Karl-Fischer titration. Spectra of the
same sample collected by four different FTIR micro spectrometers vary
by up to 10% relative in peak intensities. The differences are attribu
ted to the specific measurement conditions (e.g., magnification of the
objectives, spectral ranges of the systems, characteristics of the de
tectors) applied in the laboratories. However, an unambiguous explanat
ion of the differences is not possible due to the complexity of FTIR s
pectroscopy. In order to reduce the uncertainty in determination of wa
ter species and total water by FTIR spectroscopy a calibration of spec
trometers against a reference system should be performed. For evaluati
on of linear and integral molar extinction coefficients we have chosen
the FTIR spectrometer Bruker(R) IFS88 of Hannover as the reference sy
stem. All spectroscopic data were recalculated on the basis of this sp
ectrometer. For compositions of the system MAlSi(3)O(8) the extinction
coefficients are strongly dependent on the alkali cation and vary non
-linearly along the binary joins of the system. The extinction coeffic
ients of both the 4500- and the 5200-cm(-1) bands are significantly lo
wer for a strong peralkaline glass than for glasses with feldspar comp
ositions. This is attributed to strong H bonding of water species to a
djacent non-bridging oxygens in the peralkaline glass, Probably, for t
he peralkaline composition only a part of the water species contribute
to the NIR absorption bands. Variation of species concentration for g
lasses of the system MAlSi(3)O(8) with same water content are attribut
ed to differences in the fictive temperature of the glass which depend
s on cooling rate, water content and anhydrous composition of glass.