Abstract:Satellite observations have tremendously advanced our understandings on the emissions, distributions, chemistry, and trends of critical atmospheric pollutants and greenhouse gases (
“…For comparison, we include TROPOMI NO 2 measurements as a tracer for primary emissions from oil and gas production. Prior studies have shown that satellite NO 2 VCDs over the Permian Basin are correlated with oil and gas production activities since the mid-2000s − and can even be used to infer oil- and gas-related NO x emissions. , The summer averages 2018/2019 for formaldehyde, NO 2 , and oil and gas production are shown in Figure a–c. Here, oil and gas production volumes are averaged on a grid that matches the satellite data.…”
Section: Resultsmentioning
confidence: 99%
“…Most production regions in the United States are in relatively remote regions, where ground-based pollution measurements are sparse or nonexistent. Satellite remote sensing data have therefore played an important role in quantifying the emissions of methane and nitrogen oxides. ,− Satellite measurements of the nonmethane hydrocarbons released from oil and gas are not available to date. What is available are measurements of formaldehyde (HCHO), which can be released as a combustion byproduct and formed in the atmosphere from the photooxidation of precursor VOCs.…”
We analyzed observational and model data to study the sources of formaldehyde over oil and gas production regions and to investigate how these observations may be used to constrain oil and gas volatile organic compound (VOC) emissions. The analysis of aircraft and satellite data consistently found that formaldehyde over oil and gas production regions during spring and summer is mostly formed by the photooxidation of precursor VOCs. Formaldehyde columns over the Permian Basin, one of the largest oil-and gasproducing regions in the United States, are correlated with the production locations. Formaldehyde simulations by the atmospheric chemistry and transport model WRF-Chem, which included oil and gas NO x and VOC emissions from the fuel-based oil and gas inventory, were in very good agreement with TROPOMI satellite measurements. Sensitivity studies illustrated that VOCs released from oil and gas activities are important precursors to formaldehyde, but other sources of VOCs contribute as well and that the formation of secondary formaldehyde is highly sensitive to NO x . We also investigated the ability of the chemical mechanism used in WRF-Chem to represent formaldehyde formation from oil and gas hydrocarbons by comparing against the Master Chemical Mechanism. Further, our work provides estimates of primary formaldehyde emissions from oil and gas production activities, with per basin averages ranging from 0.07 to 2.2 kg h −1 in 2018. A separate estimate for natural gas flaring found that flaring emissions could contribute 5 to 12% to the total primary formaldehyde emissions for the Permian Basin in 2018.
“…For comparison, we include TROPOMI NO 2 measurements as a tracer for primary emissions from oil and gas production. Prior studies have shown that satellite NO 2 VCDs over the Permian Basin are correlated with oil and gas production activities since the mid-2000s − and can even be used to infer oil- and gas-related NO x emissions. , The summer averages 2018/2019 for formaldehyde, NO 2 , and oil and gas production are shown in Figure a–c. Here, oil and gas production volumes are averaged on a grid that matches the satellite data.…”
Section: Resultsmentioning
confidence: 99%
“…Most production regions in the United States are in relatively remote regions, where ground-based pollution measurements are sparse or nonexistent. Satellite remote sensing data have therefore played an important role in quantifying the emissions of methane and nitrogen oxides. ,− Satellite measurements of the nonmethane hydrocarbons released from oil and gas are not available to date. What is available are measurements of formaldehyde (HCHO), which can be released as a combustion byproduct and formed in the atmosphere from the photooxidation of precursor VOCs.…”
We analyzed observational and model data to study the sources of formaldehyde over oil and gas production regions and to investigate how these observations may be used to constrain oil and gas volatile organic compound (VOC) emissions. The analysis of aircraft and satellite data consistently found that formaldehyde over oil and gas production regions during spring and summer is mostly formed by the photooxidation of precursor VOCs. Formaldehyde columns over the Permian Basin, one of the largest oil-and gasproducing regions in the United States, are correlated with the production locations. Formaldehyde simulations by the atmospheric chemistry and transport model WRF-Chem, which included oil and gas NO x and VOC emissions from the fuel-based oil and gas inventory, were in very good agreement with TROPOMI satellite measurements. Sensitivity studies illustrated that VOCs released from oil and gas activities are important precursors to formaldehyde, but other sources of VOCs contribute as well and that the formation of secondary formaldehyde is highly sensitive to NO x . We also investigated the ability of the chemical mechanism used in WRF-Chem to represent formaldehyde formation from oil and gas hydrocarbons by comparing against the Master Chemical Mechanism. Further, our work provides estimates of primary formaldehyde emissions from oil and gas production activities, with per basin averages ranging from 0.07 to 2.2 kg h −1 in 2018. A separate estimate for natural gas flaring found that flaring emissions could contribute 5 to 12% to the total primary formaldehyde emissions for the Permian Basin in 2018.
“…Other work also demonstrates that some regions of negative emission estimated via the divergence method in the Permian can be related to changes in orogoraphy, surface albedo, or convergent wind fields [28]. Other works demonstrate that timeaveraged emission calculations from the divergence method are unlikely to be dominated by convergent wind fields [27], and other formulations of the divergence method calculate advective flux without any contribution from wind field divergence [48,49]. One could develop a model that prohibits the estimation of negative methane emissions (other works do so in a Bayesian framework [17,50]), though at this stage this would no longer purely be the 'divergence method' , which is driven entirely by the data and the principle of the conservation of mass.…”
Methane is a powerful greenhouse gas, and a primary target for mitigating climate change in the short-term future due to its relatively short atmospheric lifetime and greater ability to trap heat in Earth's atmosphere compared to carbon dioxide. Top-down observations of atmospheric methane are possible via drone and aircraft surveys as well as satellites such as the TROPOspheric Monitoring Instrument (TROPOMI). Recent work has begun to apply the divergence method to produce regional methane emission rate estimates. Here we show that when the divergence method is applied to spatially incomplete observations of methane, it can result in negatively biased time-averaged regional emission rates. We show that this effect can be counteracted by adopting a procedure in which daily advective fluxes of methane are time-averaged before the divergence method is applied. Using such a procedure with TROPOMI methane observations, we calculate yearly Permian emission rates of 3.1, 2.4 and 2.7 million tonnes per year for the years 2019 through 2021. We also show that highly-resolved plumes of methane can have negatively biased estimated emission rates by the divergence method due to the presence of turbulent diffusion in the plume, but this is unlikely to affect regional methane emission budgets constructed from TROPOMI observations of methane. The results from this work are expected to provide useful guidance for future implementations of the divergence method for emission rate estimation from satellite data -- be it for methane or other gaseous species in the atmosphere.
“…The divergence method has mainly been applied to TROPOMI data (primarily NO 2 , but also CO and CH 4 data (e.g., Beirle et al, 2019Beirle et al, , 2021Beirle et al, , 2023Liu et al, 2021;de Foy & Schauer, 2022;Sun, 2022;Rey-Pommier et al, 2022, 2023Dix et al, 2022;Filonchyk & Peterson, 2023;Lonsdale & Sun, 2023). Recently, the method has also been applied to other satellites such as GEMS NO 2 data (Xu et al, 2023).…”
Section: Introductionmentioning
confidence: 99%
“…A study of its application to synthetic CO 2 data for the upcoming CO2M mission can be found in Hakkarainen et al (2022), which notes that a background and noise removal step must be applied to make the method robust for CO 2 data. Since its inception by Beirle et al (2019), notable improvements to the method include a different order of operations (differentiatethen-average instead of average-then-differentiate) as proposed in de Foy and Schauer (2022), computing the results on the satellite swaths themselves before remapping to a uniform grid as proposed in de Foy and Schauer (2022), skipping computations proportional to the wind divergence and adding a correction term proportional to the gradient of the topography as proposed in Sun (2022), and approximating the divergence operation using finite-difference stencils that can account for non-pixel-aligned transport as proposed in Sun (2022) and Veefkind et al (2023).…”
The divergence method, a lightweight approach for estimating emission
fluxes from satellite images, relies on a number of tacit assumptions.
This paper explicitly outlines these assumptions by deriving the method
from first principles. The assumptions are: the enhanced mass flux is
dominated by advection, normal fluxes vanish at the top and bottom of
the atmosphere, steady-state conditions apply, sources are
multiplications of temporal and spatial functions, sinks are described
as first-order reactions, and effective wind fields are made by weighing
the fields with the enhanced concentration profiles. No such assumptions
have to be assumed for the background field. The commonly used
‘topography correction term’ does not follow from this analysis and
likely corrects data artifacts. The cross-sectional flux method follows
naturally from the derived theory, and the methods are compared. Effects
of discrete pixels and finite-difference operations are explored,
leading to recommendations, primarily the recommendation to work with
small regions only to minimize the influence of noise. Numerical
examples featuring Gaussian plume and COSMO-GHG simulated plumes are
provided. The Gaussian plume example suggests that the divergence method
might underestimate emissions when assuming only advection in the
presence of cross-wind diffusion. Conversely, the cross-sectional flux
method remains unaffected, provided fluxes are integrated across the
entire plume. The COSMO-GHG example reveals frequent violations of
steady-state assumption, although the assumption remains valid proximal
to the source (<20 km in this example). It is the hope that
this paper provides a solid theoretical foundation for the divergence
and cross-sectional flux methods.
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