Background heterogeneity and other uncertainties in estimating urban methane flux: results from the Indianapolis Flux Experiment (INFLUX)
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Published:2020-04-17
Issue:7
Volume:20
Page:4545-4559
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ISSN:1680-7324
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Container-title:Atmospheric Chemistry and Physics
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language:en
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Short-container-title:Atmos. Chem. Phys.
Author:
Balashov Nikolay V., Davis Kenneth J.ORCID, Miles Natasha L.ORCID, Lauvaux ThomasORCID, Richardson Scott J., Barkley Zachary R., Bonin Timothy A.
Abstract
Abstract. As natural gas extraction and use continues to increase, the need to
quantify emissions of methane (CH4), a powerful greenhouse gas, has
grown. Large discrepancies in Indianapolis CH4 emissions have been
observed when comparing inventory, aircraft mass balance, and tower inverse
modeling estimates. Four years of continuous CH4 mole fraction
observations from a network of nine towers as a part of the Indianapolis
Flux Experiment (INFLUX) are utilized to investigate four possible reasons
for the abovementioned inconsistencies: (1) differences in definition of the
city domain, (2) a highly temporally variable and spatially non-uniform
CH4 background, (3) temporal variability in CH4 emissions, and (4) CH4 sources that are not accounted for in the inventory. Reducing the
Indianapolis urban domain size to be consistent with the inventory domain
size decreases the CH4 emission estimation of the inverse modeling
methodology by about 35 %, thereby lessening the discrepancy and bringing
total city flux within the error range of one of the two inventories.
Nevertheless, the inverse modeling estimate still remains about 91 %
higher than inventory estimates. Hourly urban background CH4 mole
fractions are shown to be spatially heterogeneous and temporally variable.
Variability in background mole fractions observed at any given moment and a
single location could be up to about 50 ppb depending on a wind direction
but decreases substantially when averaged over multiple days. Statistically
significant, long-term biases in background mole fractions of 2–5 ppb are
found from single-point observations for most wind directions. Boundary
layer budget estimates suggest that Indianapolis CH4 emissions did not
change significantly when comparing 2014 to 2016. However, it appears that
CH4 emissions may follow a diurnal cycle, with daytime emissions (12:00–16:00 LST) approximately twice as large as nighttime emissions (20:00–05:00 LST). We
found no evidence for large CH4 point sources that are otherwise
missing from the inventories. The data from the towers confirm that the
strongest CH4 source in Indianapolis is South Side landfill. Leaks from
the natural gas distribution system that were detected with the tower
network appeared localized and non-permanent. Our simple atmospheric budget
analyses estimate the magnitude of the diffuse natural gas source to be 70 % higher
than inventory estimates, but more comprehensive analyses are needed.
Long-term averaging, spatially extensive upwind mole fraction observations,
mesoscale atmospheric modeling of the regional emissions environment, and
careful treatment of the times of day are recommended for precise and
accurate quantification of urban CH4 emissions.
Funder
National Institute of Standards and Technology
Publisher
Copernicus GmbH
Subject
Atmospheric Science
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