posted on 2018-12-19, 00:00authored byJ. David Felix, Rachel Thomas, Matt Casas, Megumi S. Shimizu, G. Brooks Avery, Robert J. Kieber, Ralph N. Mead, Chad S. Lane, Joan D. Willey, Amanda Guy, M. Lucia A. M. Campos
Global
atmospheric ethanol budget models include large uncertainties
in the magnitude of ethanol emission sources and sinks. To apply stable
isotope techniques to constrain ethanol emission sources, a headspace
solid phase microextraction gas chromatograph-combustion-isotope ratio
mass spectrometry method (HS-SPME-GC-C-IRMS) was developed to measure
the carbon isotopic composition of aqueous phase ethanol at natural
abundance levels (1–30 μM) with a precision of 0.4‰.
The method was applied to determine the carbon isotope signatures
(δ13C) of vehicle ethanol emission sources in Brazil
(−12.8 ± 2.4‰) and the US (−9.8 ± 2.5‰),
and to measure the carbon isotope composition of ethanol in wet deposition
(−22.6 to −12.7‰). A two end-member isotope mixing
model was developed using anthropogenic and biogenic end members and
fractionation scenarios to estimate ethanol source contributions to
wet deposition collected in Brazil and US. Mixing model results indicate
anthropogenic sources contribute two and a half to four times more
ethanol to the atmosphere than previously predicted in modeled global
ethanol inventories. As established and developing countries continue
to rapidly increase ethanol fuel consumption and subsequent emissions,
understanding the magnitude of all ethanol sources and sinks will
be essential for modeling future atmospheric chemistry and air quality
impacts.