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Applications of eddy covariance flux
measurements in quantifying whole-
city urban GHG emissions
Kenneth Davis1, Natasha Miles1, Scott Richardson1, Alex Zhang1, Samantha Murphy1,
Jason Horne1, Claire Jin2, Kai Wu3, Sharon Gourdji4, Kevin Gurney5, Geoffrey Roest5,
Jocelyn Turnbull6
1The Pennsylvania State University, University Park, USA. 2Carnegie Mellon University,
Pittsburgh, USA. 3Edinburgh University, Edinburgh, United Kingdom. 4National
Institute for Standards and Technology, Gaithersburg, USA. 5Northern Arizona
University, Flagstaff, USA. 6GNS Science, Lower Hutt, New Zealand
ICOS
Picarro cavity
ring-down
spectrometer and
calibration tank.
Continuous
measurements of GHG
Urban GHG emissions studies in the US rely primarily on
atmospheric inversions
Measure GHG
enhancements caused by
urban fluxes (Miles et al.,
2017).
Solve for emissions using
atmospheric budgets
(Heimburger et al.,
2017); or inversions
(Lauvaux et al, 2020).
Communications
tower
Maps courtesy of Vanessa Monteiro
Red cities are NIST urban test-beds
What about flux towers?
How can they be used to complement urban GHG studies?
Urban eddy covariance: Why?
• Same purpose as rural flux towers. Develop, evaluate and improve
process-based flux models that we can then extrapolate over space
and time.
• Measure fluxes continuously, and at high resolution in space and time.
• Collect ancillary data required to test process-level understanding.
• But some urban flux measurements require modifications to the
traditional ecosystem flux tower deployment.
Objectives
• Evaluate our process-level understanding of anthropogenic GHG
emissions (e.g. Gurney et al, 2012) with observations.
• Calibrate/test our models of ecosystem GHG fluxes within the city.
• Calibrate/test our models of ecosystem GHG fluxes outside of the city.
Objectives
• Evaluate our process-level understanding of anthropogenic GHG
emissions (e.g. Gurney et al, 2012) with observations.
• Calibrate/test our models of ecosystem GHG fluxes within the city.
• Calibrate/test our models of ecosystem GHG fluxes outside of the city.
Decomposition of flux measurements: Essential for heterogeneous environments
Distance to the site (m)
90%
80%
70%
-800 -400 0 400 800
800
400
0
-400
-800
Flux footprint at tower 2
• Mixed suburban
environment
• Communications
tower
• Three-level
CO/CO2/CH4
profile (10, 40,
136m AGL)
• Flux
instrumentation
at 30 m AGL
• Flux system
operated for
about seven
months.
Wu et al, 2002.
Cold season (JFM):
traffic emissions and
domestic heating
Warm season (AMJJ):
photosynthesis,
respiration,
and CO2ff emissions.
Total CO2 fluxes look very
reasonable in time:
● Traffic peaks at rush hours
● Biological flux contributions
in the summer.
Cold season (JFM) Warm season (AMJJ)
And in space:
● Fluxes are large and positive from the
north (highway), and
● smaller, sometimes negative from the
south (suburban, vegetation).
Flux data show expected patterns for mixed biological and
anthropogenic CO2 fluxes
● But these are total CO2 fluxes. We can’t compare these directly to
our models.
● We can do better…
● We decompose fluxes into biological and anthropogenic
components using CO/CO2 ratios calibrated by 14CO2,
● and decompose the fluxes in space using a flux footprint model to
match our “bottom up” models” pixel by pixel.
● Then we can construct “apples to apples” tests of our “bottom-up”
modeling systems
Methods: disaggregate fossil fuel and biogenic CO2 fluxes using trace gases
^ ^
^ ^
^
^
^
Assumption:
• CO and CO2 have similar vertical mixing
process (same eddy diffusivity)
Data screening:
• No counter gradient flux (K > 0)
• No negative CO flux (delta CO > 0)
• K and FCO are smaller than 3.5 σ
9
Use 14CO2 to evaluate the
CO/CO2ff ratio (R).
Downwind – upwind
CO/CO2ff ratio from flasks
defines R. Select R = 9 ppb
/ ppm.
Flux decomposition yields fossil and bio CO2 fluxes
Cold season (JFM) Warm season (AMJJ)
Photosynthesis in the winter?
(b)
CO2 flux
(µmol m-2 s-
1)
Match every half-hourly flux footprint in space to the Hestia emissions map
Annual mean of high-resolution (200m) Hestia emissions inventory
• Hestia! Gurney et al., (2012).
• High spatial and temporal
resolution cousin of Vulcan –
anthropogenic CO2 emissions
model / inventory / data product.
• Hourly temporal resolution.
• 200 m spatial resolution.
• Integrates a wide variety of activity
and inventory data.
• Only available for a few cities and
years. Lots of work to create!
• NEVER BEEN TESTED at high spatial
and temporal resolution (until
now).
Note: emissions are limited to 20 µmol m-2 s-1 for visualization.
(a)
(b)
CO2 flux
(µmol m-2 s-
1)
Match every half-hourly flux footprint in space to the Hestia emissions map
Flux footprint from one half-hourly data
Distance to the site (m)
• Flux footprint is related to instrument height,
atmospheric stability and surface roughness.
• Tower measurements were used to calculate
input parameters of flux footprint model.
Annual mean of high-resolution (200m) Hestia emissions inventory
• Hestia has fine-scale spatial structure in urban CO2
emissions, complementary to flux data.
• High emissions are correlated to the distribution of roads.
Note: emissions are limited to 20 µmol m-2 s-1 for visualization.
Hestia - Eddy Covariance bias and temporal pattern comparisons
Very small percentage bias (3%, 9%) in
the seasonal averaged CO2ff emissions.
Modest RMSE, probably dominated by
sampling error from the eddy
covariance methods.
Shockingly close agreement in the
seasonal temporal pattern of CO2ff
emissions.
Wu et al, 2022
Impressive agreement in the spatial pattern of emissions: Some suggestion for
differences in home heating emissions
Hestia emissions
are higher than the
observed CO2ff
emissions for the
“non-traffic” wind
directions.
See, for example, E,
SE, S wind
directions in the
cold season.
Since residential
buildings lie upwind
in these directions,
residential
emissions may be
the source of this
discrepancy.
Wu et al, 2022
What are the implications of this comparison?
● For a first high-resolution (space and time) comparison between
model and data, this is encouraging. Hestia takes a lot of work to
create, but it appears to work very well.
● This flux decomposition approach also appears to work well.
● This lends confidence in our ability to deploy and use flux towers to
construct additional detailed evaluation of our models of
anthropogenic emissions.
● We don’t yet have a very high-resolution urban ecosystem model to
test.
Objectives
• Evaluate our process-level understanding of anthropogenic GHG
emissions (e.g. Gurney et al, 2012) with observations.
• Calibrate/test our models of ecosystem GHG fluxes within the city.
• Calibrate/test our models of ecosystem GHG fluxes outside of the city.
Flux decomposition yields fossil and bio CO2 fluxes
Cold season (JFM) Warm season (AMJJ)
Photosynthesis in the winter?
Next: Watching the grass grow...
CO
2
flux
(µmol
m
-2
s
-1
)
Hour (LST)
Winter (November to December in 2017)
● Turf grass within the city shows large daytime fluxes (-8 µmol m-2 s-1) in the dormant season.
● This daytime flux density magnitude is comparable to fossil fuel emissions.
● First assumptions have been to ignore biology for dormant season atmospheric inversions.
● Current ecosystem model parameters aren’t adapted to turf grass.
Summer (June to August in 2018)
Hour (LST)
CO
2
flux
(µmol
m
-2
s
-1
)
Turf grass is very active in the dormant season!
Photosynthesis in the winter!
Turf grass coverage
is substantial.
Should it be a
separate plant
functional type in a
simple urban
ecosystem model like
VPRM?
Horne et al, in prep
Optimize VPRM parameters with flux
observations - create a turf grass PFT
Compare to a prior version of VPRM which used deciduous broadleaf forest for all urban vegetation.
Horne et al, in prep
Midday winter (3 January, 2019) simulated NEE changes dramatically
when a turf grass PFT is used
Previous version of
VPRM (urban
vegetation = DBF)
overestimates
midday, winter NEE
across this domain
by about 2000 mol
s-1, approximately
10% of urban
anthropogenic
emissions from
Indianapolis.
Urban vegetation = DBF
Crops and DBF surround the city
Urban vegetation = DBF + turfgrass
Crops and DBF surround the city Horne et al, in prep
Objectives
• Evaluate our process-level understanding of anthropogenic GHG
emissions (e.g. Gurney et al, 2012) with observations.
• Calibrate/test our models of ecosystem GHG fluxes within the city.
• Calibrate/test our models of ecosystem GHG fluxes outside of the city.
• Why is this important?
Why do agricultural fluxes matter when studying
urban anthropogenic GHG emissions?
Miles et al., (2021)
Map shows mole fraction towers. 01, 09 and 14 are “background” towers.
Why do agricultural fluxes matter when studying
urban anthropogenic GHG emissions?
Miles et al., (2021)
• Summer rural biogenic draw-down
causes large afternoon
enhancements. Rural fluxes must be
accounted for to isolate urban GHG
emissions.
• Growing season differences among
“background” mole fraction
observations can be the same order
of magnitude as urban GHG
enhancements.
• We need regional flux tower data to
create a solid understanding of the
variations in the rural CO2
background.
Inset shows mole fraction towers. 01, 09 and 14 are “background” towers.
Testing is underway
Vegetation Photosynthesis
Respiration Model VPRM runs
for a 300 x 300 km2 grid
around Indianapolis
Compare VPRM CO2 flux outputs to
agricultural eddy covariance
measurements
- Does VPRM represent flux
measurements? (If no, optimize)
Convolve VPRM CO2 flux outputs with CO2
concentration tower influence functions
- Does VPRM explain the background
mole fraction differences observed in
Miles et al., (2021)?
Use VPRM to represent rural background conditions for Urban Inversions
Murphy et al, in prep
Conclusions
● Urban flux towers can be used, with appropriate data decomposition
methods and tower placement strategies, for direct, quantitative tests of
urban anthropogenic and biogenic flux models.
● This work complements urban anthropogenic GHG inversions by
● Improving our understanding of the biogenic GHG flux environment (urban and
rural).
● Evaluating our anthropogenic emissions “priors” at high spatial and temporal
resolution – potentially identifying process errors in those priors and eliminating
those errors.
● Improving our models of surface energy and momentum fluxes needed for
atmospheric transport models.
References
Gurney, K.R., et al. (2012). Quantification of Fossil Fuel CO2 Emissions on the Building/Street Scale for a Large U.S. City. Environ. Sci. Technol., 46, 21, 12194–
12202. https://doi.org/10.1021/es3011282.
Heimberger, Alexie M. F., Paul B. Shepson, Brian H. Stirm, Chloe Susdorf, Jocelyn Turnbull, Maria O. L. Cambaliza, Olivia E. Salmon, Anna-Elodie M. Kerlo, Tegan N.
Lavoie, Rebecca M. Harvey, Kenneth J. Davis, Thomas Lauvaux, Anna Karion, Colm Sweeney, W. Allen Brewer, R. Michael Hardesty, Kevin R. Gurney, James
Whetstone, 2017. Precision Assessment for the Aircraft Mass Balance Method for Measurement of Urban Greenhouse Gas Emission Rates. Elem Sci Anth.
2017;5:26. DOI: http://doi.org/10.1525/elementa.134
Lauvaux, T., K.R. Gurney, N.L. Miles, K.J. Davis, S.J. Richardson, A. Deng, B.J. Nathan, T. Oda, J.A.Wang, L.R. Hutyra, and J.C.Turnbull, 2020. Policy-relevant
assessment of urban greenhouse gas emissions, Environ Sci Tech. 54, 16, 10237–10245, doi:10.1021/acs.est.0c00343.
Miles, Natasha L., Kenneth J. Davis, Scott J. Richardson, Thomas Lauvaux, Douglas K. Martins, A. J. Deng, Nikolay Balashov, Kevin R. Gurney, Jianming Liang, Geoff
Roest, Jonathan A. Wang, 2021: The influence of near-field fluxes on seasonal carbon dioxide enhancements: results from the Indianapolis Flux Experiment
(INFLUX). Carbon Balance and Management, 16:4, https://doi.org/10.1186/s13021-020-00166-z
Miles, Natasha L., Scott J. Richardson, Thomas Lauvaux, Kenneth J. Davis, Aijun Deng, Jocelyn Turnbull, Anna Karion, Colm Sweeney, Kevin R. Gurney, Risa
Patarasuk, Igor Razlivanov, Maria O. Cambaliza and Paul B. Shepson, 2017. Quantification of urban atmospheric boundary layer greenhouse gas dry mole fraction
enhancements: Results from the Indianapolis Flux Experiment (INFLUX), Elem Sci Anth. 2017;5:27. DOI: http://doi.org/10.1525/elementa.127
Turnbull, Jocelyn C., Anna Karion, Kenneth J. Davis, Thomas Lauvaux, Natasha L. Miles, Scott J. Richardson, Colm Sweeney, Kathryn McKain, Scott J. Lehman, Kevin
R. Gurney, Risa Patarasuk, Jianming Liang, Paul B. Shepson, Alexie Heimburger, Rebecca Harvey, and James Whetstone, 2019. Synthesis of Urban CO2 Emission
Estimates from Multiple Methods from the Indianapolis Flux Project (INFLUX). Environmental Science & Technology 2019 53 (1), 287-295,
DOI:10.1021/acs.est.8b05552.
Wu, Kai, Kenneth J Davis, Natasha L Miles, Scott J Richardson, Thomas Lauvaux, Daniel P Sarmiento, Nikolay V Balashov, Klaus Keller, Jocelyn Turnbull, Kevin R
Gurney, Jianming Liang and Geoffrey Roest, 2022. Source decomposition of eddy-covariance CO2 flux measurements for evaluating a high-resolution urban CO2
emissions inventory, Environ. Res. Lett. 17 074035, https://doi.org/10.1088/1748-9326/ac7c29

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Davis, Kenneth: Applications of eddy covariance flux measurements in quantifying whole-city urban GHG emissions

  • 1. Applications of eddy covariance flux measurements in quantifying whole- city urban GHG emissions Kenneth Davis1, Natasha Miles1, Scott Richardson1, Alex Zhang1, Samantha Murphy1, Jason Horne1, Claire Jin2, Kai Wu3, Sharon Gourdji4, Kevin Gurney5, Geoffrey Roest5, Jocelyn Turnbull6 1The Pennsylvania State University, University Park, USA. 2Carnegie Mellon University, Pittsburgh, USA. 3Edinburgh University, Edinburgh, United Kingdom. 4National Institute for Standards and Technology, Gaithersburg, USA. 5Northern Arizona University, Flagstaff, USA. 6GNS Science, Lower Hutt, New Zealand ICOS
  • 2. Picarro cavity ring-down spectrometer and calibration tank. Continuous measurements of GHG Urban GHG emissions studies in the US rely primarily on atmospheric inversions Measure GHG enhancements caused by urban fluxes (Miles et al., 2017). Solve for emissions using atmospheric budgets (Heimburger et al., 2017); or inversions (Lauvaux et al, 2020). Communications tower Maps courtesy of Vanessa Monteiro Red cities are NIST urban test-beds What about flux towers? How can they be used to complement urban GHG studies?
  • 3. Urban eddy covariance: Why? • Same purpose as rural flux towers. Develop, evaluate and improve process-based flux models that we can then extrapolate over space and time. • Measure fluxes continuously, and at high resolution in space and time. • Collect ancillary data required to test process-level understanding. • But some urban flux measurements require modifications to the traditional ecosystem flux tower deployment.
  • 4. Objectives • Evaluate our process-level understanding of anthropogenic GHG emissions (e.g. Gurney et al, 2012) with observations. • Calibrate/test our models of ecosystem GHG fluxes within the city. • Calibrate/test our models of ecosystem GHG fluxes outside of the city.
  • 5. Objectives • Evaluate our process-level understanding of anthropogenic GHG emissions (e.g. Gurney et al, 2012) with observations. • Calibrate/test our models of ecosystem GHG fluxes within the city. • Calibrate/test our models of ecosystem GHG fluxes outside of the city.
  • 6. Decomposition of flux measurements: Essential for heterogeneous environments Distance to the site (m) 90% 80% 70% -800 -400 0 400 800 800 400 0 -400 -800 Flux footprint at tower 2 • Mixed suburban environment • Communications tower • Three-level CO/CO2/CH4 profile (10, 40, 136m AGL) • Flux instrumentation at 30 m AGL • Flux system operated for about seven months. Wu et al, 2002.
  • 7. Cold season (JFM): traffic emissions and domestic heating Warm season (AMJJ): photosynthesis, respiration, and CO2ff emissions. Total CO2 fluxes look very reasonable in time: ● Traffic peaks at rush hours ● Biological flux contributions in the summer. Cold season (JFM) Warm season (AMJJ) And in space: ● Fluxes are large and positive from the north (highway), and ● smaller, sometimes negative from the south (suburban, vegetation). Flux data show expected patterns for mixed biological and anthropogenic CO2 fluxes
  • 8. ● But these are total CO2 fluxes. We can’t compare these directly to our models. ● We can do better… ● We decompose fluxes into biological and anthropogenic components using CO/CO2 ratios calibrated by 14CO2, ● and decompose the fluxes in space using a flux footprint model to match our “bottom up” models” pixel by pixel. ● Then we can construct “apples to apples” tests of our “bottom-up” modeling systems
  • 9. Methods: disaggregate fossil fuel and biogenic CO2 fluxes using trace gases ^ ^ ^ ^ ^ ^ ^ Assumption: • CO and CO2 have similar vertical mixing process (same eddy diffusivity) Data screening: • No counter gradient flux (K > 0) • No negative CO flux (delta CO > 0) • K and FCO are smaller than 3.5 σ 9 Use 14CO2 to evaluate the CO/CO2ff ratio (R). Downwind – upwind CO/CO2ff ratio from flasks defines R. Select R = 9 ppb / ppm.
  • 10. Flux decomposition yields fossil and bio CO2 fluxes Cold season (JFM) Warm season (AMJJ) Photosynthesis in the winter?
  • 11. (b) CO2 flux (µmol m-2 s- 1) Match every half-hourly flux footprint in space to the Hestia emissions map Annual mean of high-resolution (200m) Hestia emissions inventory • Hestia! Gurney et al., (2012). • High spatial and temporal resolution cousin of Vulcan – anthropogenic CO2 emissions model / inventory / data product. • Hourly temporal resolution. • 200 m spatial resolution. • Integrates a wide variety of activity and inventory data. • Only available for a few cities and years. Lots of work to create! • NEVER BEEN TESTED at high spatial and temporal resolution (until now). Note: emissions are limited to 20 µmol m-2 s-1 for visualization.
  • 12. (a) (b) CO2 flux (µmol m-2 s- 1) Match every half-hourly flux footprint in space to the Hestia emissions map Flux footprint from one half-hourly data Distance to the site (m) • Flux footprint is related to instrument height, atmospheric stability and surface roughness. • Tower measurements were used to calculate input parameters of flux footprint model. Annual mean of high-resolution (200m) Hestia emissions inventory • Hestia has fine-scale spatial structure in urban CO2 emissions, complementary to flux data. • High emissions are correlated to the distribution of roads. Note: emissions are limited to 20 µmol m-2 s-1 for visualization.
  • 13. Hestia - Eddy Covariance bias and temporal pattern comparisons Very small percentage bias (3%, 9%) in the seasonal averaged CO2ff emissions. Modest RMSE, probably dominated by sampling error from the eddy covariance methods. Shockingly close agreement in the seasonal temporal pattern of CO2ff emissions. Wu et al, 2022
  • 14. Impressive agreement in the spatial pattern of emissions: Some suggestion for differences in home heating emissions Hestia emissions are higher than the observed CO2ff emissions for the “non-traffic” wind directions. See, for example, E, SE, S wind directions in the cold season. Since residential buildings lie upwind in these directions, residential emissions may be the source of this discrepancy. Wu et al, 2022
  • 15. What are the implications of this comparison? ● For a first high-resolution (space and time) comparison between model and data, this is encouraging. Hestia takes a lot of work to create, but it appears to work very well. ● This flux decomposition approach also appears to work well. ● This lends confidence in our ability to deploy and use flux towers to construct additional detailed evaluation of our models of anthropogenic emissions. ● We don’t yet have a very high-resolution urban ecosystem model to test.
  • 16. Objectives • Evaluate our process-level understanding of anthropogenic GHG emissions (e.g. Gurney et al, 2012) with observations. • Calibrate/test our models of ecosystem GHG fluxes within the city. • Calibrate/test our models of ecosystem GHG fluxes outside of the city.
  • 17. Flux decomposition yields fossil and bio CO2 fluxes Cold season (JFM) Warm season (AMJJ) Photosynthesis in the winter?
  • 18. Next: Watching the grass grow...
  • 19. CO 2 flux (µmol m -2 s -1 ) Hour (LST) Winter (November to December in 2017) ● Turf grass within the city shows large daytime fluxes (-8 µmol m-2 s-1) in the dormant season. ● This daytime flux density magnitude is comparable to fossil fuel emissions. ● First assumptions have been to ignore biology for dormant season atmospheric inversions. ● Current ecosystem model parameters aren’t adapted to turf grass. Summer (June to August in 2018) Hour (LST) CO 2 flux (µmol m -2 s -1 ) Turf grass is very active in the dormant season! Photosynthesis in the winter!
  • 20. Turf grass coverage is substantial. Should it be a separate plant functional type in a simple urban ecosystem model like VPRM? Horne et al, in prep
  • 21. Optimize VPRM parameters with flux observations - create a turf grass PFT Compare to a prior version of VPRM which used deciduous broadleaf forest for all urban vegetation. Horne et al, in prep
  • 22. Midday winter (3 January, 2019) simulated NEE changes dramatically when a turf grass PFT is used Previous version of VPRM (urban vegetation = DBF) overestimates midday, winter NEE across this domain by about 2000 mol s-1, approximately 10% of urban anthropogenic emissions from Indianapolis. Urban vegetation = DBF Crops and DBF surround the city Urban vegetation = DBF + turfgrass Crops and DBF surround the city Horne et al, in prep
  • 23. Objectives • Evaluate our process-level understanding of anthropogenic GHG emissions (e.g. Gurney et al, 2012) with observations. • Calibrate/test our models of ecosystem GHG fluxes within the city. • Calibrate/test our models of ecosystem GHG fluxes outside of the city. • Why is this important?
  • 24. Why do agricultural fluxes matter when studying urban anthropogenic GHG emissions? Miles et al., (2021) Map shows mole fraction towers. 01, 09 and 14 are “background” towers.
  • 25. Why do agricultural fluxes matter when studying urban anthropogenic GHG emissions? Miles et al., (2021) • Summer rural biogenic draw-down causes large afternoon enhancements. Rural fluxes must be accounted for to isolate urban GHG emissions. • Growing season differences among “background” mole fraction observations can be the same order of magnitude as urban GHG enhancements. • We need regional flux tower data to create a solid understanding of the variations in the rural CO2 background. Inset shows mole fraction towers. 01, 09 and 14 are “background” towers.
  • 26. Testing is underway Vegetation Photosynthesis Respiration Model VPRM runs for a 300 x 300 km2 grid around Indianapolis Compare VPRM CO2 flux outputs to agricultural eddy covariance measurements - Does VPRM represent flux measurements? (If no, optimize) Convolve VPRM CO2 flux outputs with CO2 concentration tower influence functions - Does VPRM explain the background mole fraction differences observed in Miles et al., (2021)? Use VPRM to represent rural background conditions for Urban Inversions Murphy et al, in prep
  • 27. Conclusions ● Urban flux towers can be used, with appropriate data decomposition methods and tower placement strategies, for direct, quantitative tests of urban anthropogenic and biogenic flux models. ● This work complements urban anthropogenic GHG inversions by ● Improving our understanding of the biogenic GHG flux environment (urban and rural). ● Evaluating our anthropogenic emissions “priors” at high spatial and temporal resolution – potentially identifying process errors in those priors and eliminating those errors. ● Improving our models of surface energy and momentum fluxes needed for atmospheric transport models.
  • 28. References Gurney, K.R., et al. (2012). Quantification of Fossil Fuel CO2 Emissions on the Building/Street Scale for a Large U.S. City. Environ. Sci. Technol., 46, 21, 12194– 12202. https://doi.org/10.1021/es3011282. Heimberger, Alexie M. F., Paul B. Shepson, Brian H. Stirm, Chloe Susdorf, Jocelyn Turnbull, Maria O. L. Cambaliza, Olivia E. Salmon, Anna-Elodie M. Kerlo, Tegan N. Lavoie, Rebecca M. Harvey, Kenneth J. Davis, Thomas Lauvaux, Anna Karion, Colm Sweeney, W. Allen Brewer, R. Michael Hardesty, Kevin R. Gurney, James Whetstone, 2017. Precision Assessment for the Aircraft Mass Balance Method for Measurement of Urban Greenhouse Gas Emission Rates. Elem Sci Anth. 2017;5:26. DOI: http://doi.org/10.1525/elementa.134 Lauvaux, T., K.R. Gurney, N.L. Miles, K.J. Davis, S.J. Richardson, A. Deng, B.J. Nathan, T. Oda, J.A.Wang, L.R. Hutyra, and J.C.Turnbull, 2020. Policy-relevant assessment of urban greenhouse gas emissions, Environ Sci Tech. 54, 16, 10237–10245, doi:10.1021/acs.est.0c00343. Miles, Natasha L., Kenneth J. Davis, Scott J. Richardson, Thomas Lauvaux, Douglas K. Martins, A. J. Deng, Nikolay Balashov, Kevin R. Gurney, Jianming Liang, Geoff Roest, Jonathan A. Wang, 2021: The influence of near-field fluxes on seasonal carbon dioxide enhancements: results from the Indianapolis Flux Experiment (INFLUX). Carbon Balance and Management, 16:4, https://doi.org/10.1186/s13021-020-00166-z Miles, Natasha L., Scott J. Richardson, Thomas Lauvaux, Kenneth J. Davis, Aijun Deng, Jocelyn Turnbull, Anna Karion, Colm Sweeney, Kevin R. Gurney, Risa Patarasuk, Igor Razlivanov, Maria O. Cambaliza and Paul B. Shepson, 2017. Quantification of urban atmospheric boundary layer greenhouse gas dry mole fraction enhancements: Results from the Indianapolis Flux Experiment (INFLUX), Elem Sci Anth. 2017;5:27. DOI: http://doi.org/10.1525/elementa.127 Turnbull, Jocelyn C., Anna Karion, Kenneth J. Davis, Thomas Lauvaux, Natasha L. Miles, Scott J. Richardson, Colm Sweeney, Kathryn McKain, Scott J. Lehman, Kevin R. Gurney, Risa Patarasuk, Jianming Liang, Paul B. Shepson, Alexie Heimburger, Rebecca Harvey, and James Whetstone, 2019. Synthesis of Urban CO2 Emission Estimates from Multiple Methods from the Indianapolis Flux Project (INFLUX). Environmental Science & Technology 2019 53 (1), 287-295, DOI:10.1021/acs.est.8b05552. Wu, Kai, Kenneth J Davis, Natasha L Miles, Scott J Richardson, Thomas Lauvaux, Daniel P Sarmiento, Nikolay V Balashov, Klaus Keller, Jocelyn Turnbull, Kevin R Gurney, Jianming Liang and Geoffrey Roest, 2022. Source decomposition of eddy-covariance CO2 flux measurements for evaluating a high-resolution urban CO2 emissions inventory, Environ. Res. Lett. 17 074035, https://doi.org/10.1088/1748-9326/ac7c29