12 research outputs found
Methane emissions from dairies in the Los Angeles Basin
We estimate the amount of methane (CH_4) emitted by the largest dairies in the southern California region by combining measurements from four mobile solar-viewing ground-based spectrometers (EM27/SUN), in situ isotopic ^(13∕12)CH_4 measurements from a CRDS analyzer (Picarro), and a high-resolution atmospheric transport simulation with a Weather Research and Forecasting model in large-eddy simulation mode (WRF-LES).
The remote sensing spectrometers measure the total column-averaged dry-air mole fractions of CH_4 and CO_2 (X_(CH)_4 and X_(CO)_2) in the near infrared region, providing information on total emissions of the dairies at Chino. Differences measured between the four EM27/SUN ranged from 0.2 to 22 ppb (part per billion) and from 0.7 to 3 ppm (part per million) for X_(CH)_4 and X_(CO)_2, respectively. To assess the fluxes of the dairies, these differential measurements are used in conjunction with the local atmospheric dynamics from wind measurements at two local airports and from the WRF-LES simulations at 111 m resolution.
Our top-down CH_4 emissions derived using the Fourier transform spectrometers (FTS) observations of 1.4 to 4.8 ppt s^(−1) are in the low end of previous top-down estimates, consistent with reductions of the dairy farms and urbanization in the domain. However, the wide range of inferred fluxes points to the challenges posed by the heterogeneity of the sources and meteorology. Inverse modeling from WRF-LES is utilized to resolve the spatial distribution of CH_4 emissions in the domain. Both the model and the measurements indicate heterogeneous emissions, with contributions from anthropogenic and biogenic sources at Chino. A Bayesian inversion and a Monte Carlo approach are used to provide the CH_4 emissions of 2.2 to 3.5 ppt s^(−1) at Chino
Evaluation of MOPITT Version 7 joint TIR-NIR XCO retrievals with TCCON
Observations of carbon monoxide (CO) from the Measurements Of Pollution In The Troposphere (MOPITT) instrument aboard the Terra spacecraft were expected to have an accuracy of 10 % prior to the launch in 1999. Here we evaluate MOPITT Version 7 joint (V7J) thermal-infrared and near-infrared (TIR–NIR) retrieval accuracy and precision and suggest ways to further improve the accuracy of the observations. We take five steps involving filtering or bias corrections to reduce scatter and bias in the data relative to other MOPITT soundings and ground-based measurements. (1) We apply a preliminary filtering scheme in which measurements over snow and ice are removed. (2) We find a systematic pairwise bias among the four MOPITT along-track detectors (pixels) on the order of 3–4 ppb with a small temporal trend, which we remove on a global scale using a temporally trended bias correction. (3) Using a small-region approximation (SRA), a new filtering scheme is developed and applied based on additional quality indicators such as the signal-to-noise ratio (SNR). After applying these new filters, the root-mean-squared error computed using the local median from the SRA over 16 years of global observations decreases from 3.84 to 2.55 ppb. (4) We also use the SRA to find variability in MOPITT retrieval anomalies that relates to retrieval parameters. We apply a bias correction to one parameter from this analysis. (5) After applying the previous bias corrections and filtering, we compare the MOPITT results with the GGG2014 ground-based Total Carbon Column Observing Network (TCCON) observations to obtain an overall global bias correction. These comparisons show that MOPITT V7J is biased high by about 6 %–8 %, which is similar to past studies using independent validation datasets on V6J. When using TCCON spectrometric column retrievals without the standard airmass correction or scaling to aircraft (WMO scale), the ground- and satellite-based observations overall agree to better than 0.5 %. GEOS-Chem data assimilations are used to estimate the influence of filtering and scaling to TCCON on global CO and tend to pull concentrations away from the prior fluxes and closer to the truth. We conclude with suggestions for further improving the MOPITT data products
Southern California megacity CO<sub>2</sub>, CH<sub>4</sub>, and CO flux estimates using ground- and space-based remote sensing and a Lagrangian model
We estimate the overall CO2, CH4, and CO
flux from the South Coast Air Basin using an inversion that couples Total
Carbon Column Observing Network (TCCON) and Orbiting Carbon Observatory-2
(OCO-2) observations, with the Hybrid Single Particle Lagrangian Integrated
Trajectory (HYSPLIT) model and the Open-source Data Inventory for
Anthropogenic CO2 (ODIAC). Using TCCON data we estimate the direct
net CO2 flux from the SoCAB to be
104 ± 26 Tg CO2 yr−1 for the study period of
July 2013–August 2016. We obtain a slightly higher estimate of
120 ± 30 Tg CO2 yr−1 using OCO-2 data. These
CO2 emission estimates are on the low end of previous work. Our net
CH4 (360 ± 90 Gg CH4 yr−1) flux estimate is
in agreement with central values from previous top-down studies going back to
2010 (342–440 Gg CH4 yr−1). CO emissions are estimated at
487 ± 122 Gg CO yr−1, much lower than previous top-down
estimates (1440 Gg CO yr−1). Given the decreasing emissions of CO,
this finding is not unexpected. We perform sensitivity tests to estimate how
much errors in the prior, errors in the covariance, different inversion
schemes, or a coarser dynamical model influence the emission estimates.
Overall, the uncertainty is estimated to be 25 %, with the largest
contribution from the dynamical model. Lessons learned here may help in
future inversions of satellite data over urban areas.</p
Differential column measurements using compact solar-tracking spectrometers
We demonstrate the use of compact solar-tracking Fourier transform spectrometers (Bruker EM27/SUN) for differential measurements of the column-averaged dry-air mole fractions of CH<sub>4</sub> and CO<sub>2</sub> within urban areas. Using Allan variance analysis, we show that the differential column measurement has a precision of 0.01 % for <i>X</i><sub>CO<sub>2</sub></sub> and <i>X</i><sub>CH<sub>4</sub></sub> with an optimum integration time of 10 min, corresponding to Allan deviations of 0.04 ppm and 0.2 ppb, respectively. The sensor system is very stable over time and after relocation across the continent. We report tests of the differential column measurement, and its sensitivity to emission sources, by measuring the downwind-minus-upwind column difference Δ<i>X</i><sub>CH<sub>4</sub></sub> across dairy farms in the Chino area, California, and using the data to verify emissions reported in the literature. Ratios of spatial column differences Δ<i>X</i><sub>CH<sub>4</sub></sub>∕Δ<i>X</i><sub>CO<sub>2</sub></sub> were observed across Pasadena within the Los Angeles basin, indicating values consistent with regional emission ratios from the literature. Our precise, rapid measurements allow us to determine significant short-term variations (5–10 min) of <i>X</i><sub>CO<sub>2</sub></sub> and <i>X</i><sub>CH<sub>4</sub></sub> and to show that they represent atmospheric phenomena.<br><br>Overall, this study helps establish a range of new applications for compact solar-viewing Fourier transform spectrometers. By accurately measuring the small differences in integrated column amounts across local and regional sources, we directly observe the mass loading of the atmosphere due to the influence of emissions in the intervening locale. The inference of the source strength is much more direct than inversion modeling using only surface concentrations and less subject to errors associated with small-scale transport phenomena
TCCON data from East Trout Lake, SK (CA), Release GGG2020.R0
The Total Carbon Column Observing Network (TCCON) is
a network of ground-based Fourier Transform Spectrometers that record direct
solar absorption spectra of the atmosphere in the near-infrared. From these
spectra, accurate and precise column-averaged abundances of atmospheric
constituents including CO2, CH4, N2O, HF, CO, H2O, and HDO, are retrieved. This
is the GGG2020 data release of observations from the TCCON station at
East Trout Lake, CanadaContact person: Wunch, Debra [email protected] available via S3 at https://renc.osn.xsede.org/ini210004tommorrell/10.14291/tccon.ggg2020.easttroutlake01.R0/</p>README.txt 0.0 GB
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TCCON data from East Trout Lake, SK (CA), Release GGG2014.R1
The Total Carbon Column Observing Network (TCCON) is a network of ground-based Fourier Transform Spectrometers that record direct solar absorption spectra of the atmosphere in the near-infrared. From these spectra, accurate and precise column-averaged abundances of atmospheric constituents including CO2, CH4, N2O, HF, CO, H2O, and HDO, are retrieved. This data set contains observations from the TCCON station East Trout Lake, SK, Canada.Contact person: Debra Wunch [email protected]
Assessment of errors and biases in retrievals of X<sub>CO<sub>2</sub></sub>, X<sub>CH<sub>4</sub></sub>, X<sub>CO</sub>, and X<sub>N<sub>2</sub>O</sub> from a 0.5 cm<sup>–1</sup> resolution solar-viewing spectrometer
Bruker™ EM27/SUN instruments are commercial mobile solar-viewing near-IR spectrometers. They show promise for expanding the global density of atmospheric column measurements of greenhouse gases and are being marketed for such applications. They have been shown to measure the same variations of atmospheric gases within a day as the high-resolution spectrometers of the Total Carbon Column Observing Network (TCCON). However, there is little known about the long-term precision and uncertainty budgets of EM27/SUN measurements. In this study, which includes a comparison of 186 measurement days spanning 11 months, we note that atmospheric variations of X<sub>gas</sub> within a single day are well captured by these low-resolution instruments, but over several months, the measurements drift noticeably. We present comparisons between EM27/SUN instruments and the TCCON using GGG as the retrieval algorithm. In addition, we perform several tests to evaluate the robustness of the performance and determine the largest sources of errors from these spectrometers. We include comparisons of X<sub>CO<sub>2</sub></sub>, X<sub>CH<sub>4</sub></sub>, X<sub>CO</sub>, and X<sub>N<sub>2</sub>O</sub>. Specifically we note EM27/SUN biases for January 2015 of 0.03, 0.75, –0.12, and 2.43 % for X<sub>CO<sub>2</sub></sub>, X<sub>CH<sub>4</sub></sub>, X<sub>CO</sub>, and X<sub>N<sub>2</sub>O</sub> respectively, with 1<i>σ</i> running precisions of 0.08 and 0.06 % for X<sub>CO<sub>2</sub></sub> and X<sub>CH<sub>4</sub></sub> from measurements in Pasadena. We also identify significant error caused by nonlinear sensitivity when using an extended spectral range detector used to measure CO and N<sub>2</sub>O
Intercomparability of X<sub>CO<sub>2</sub></sub> and X<sub>CH<sub>4</sub></sub> from the United States TCCON sites
The Total Carbon Column Observing Network (TCCON) has
become the standard for long-term column-averaged measurements of CO2
and CH4. Here, we use a pair of portable spectrometers to test for
intra-network bias among the four currently operating TCCON sites in the
United States (US). A previous analytical error analysis has suggested
that the maximum 2σ site-to-site relative (absolute) bias of TCCON
should be less than 0.2 % (0.8 ppm) in XCO2 and 0.4 % (7 ppb) in
XCH4. We find here experimentally that the 95 % confidence intervals
for maximum pairwise site-to-site bias among the four US TCCON sites are
0.05–0.14 % for XCO2 and 0.08–0.24 % for XCH4. This is
close to the limit of the bias we can detect using this methodology
Quantifying the loss of processed natural gas within California's South Coast Air Basin using long-term measurements of ethane and methane
Methane emissions inventories for Southern California's South Coast Air Basin (SoCAB)
have underestimated emissions from atmospheric measurements. To provide
insight into the sources of the discrepancy, we analyze records of
atmospheric trace gas total column abundances in the SoCAB starting in the
late 1980s to produce annual estimates of the ethane emissions from
1989 to 2015 and methane emissions from 2007 to 2015. The first decade of
measurements shows a rapid decline in ethane emissions coincident with
decreasing natural gas and crude oil production in the basin. Between 2010
and 2015, however, ethane emissions have grown gradually from about
13 ± 5 to about 23 ± 3 Gg yr−1, despite the steady
production of natural gas and oil over that time period. The methane
emissions record begins with 1 year of measurements in 2007 and continuous
measurements from 2011 to 2016 and shows little trend over time, with an
average emission rate of 413 ± 86 Gg yr−1. Since 2012, ethane to
methane ratios in the natural gas withdrawn from a storage facility within
the SoCAB have been increasing by 0.62 ± 0.05 % yr−1,
consistent with the ratios measured in the delivered gas. Our atmospheric
measurements also show an increase in these ratios but with a slope of
0.36 ± 0.08 % yr−1, or 58 ± 13 % of the slope
calculated from the withdrawn gas. From this, we infer that more than half of
the excess methane in the SoCAB between 2012 and 2015 is attributable to losses
from the natural gas infrastructure