Arising from Zhang et al. Nature Communications (https://doi.org/10.1038/s41467-019-14155-5) (2020)
In a recent study, Zhang et al.1 found paddy rice area and growth were strongly correlated with CH4 column-averaged dry-air mole fractions (XCH4) observed from satellites in Monsoon Asia. Based on these correlations, they argued that the spatial area and growth cycle of paddy rice drive the spatial distribution and seasonality of XCH4 in the region of the rice paddies. Here, by reanalyzing satellite XCH4 observations and running CH4 simulations with a chemical transport model, we show that (1) local variation in XCH4 is primarily driven by large scale CH4 flux signals advected into the local area rather than from local emission, indicating that variations in XCH4 do not simply translate to variations in the underlying rice paddy emissions. (2) Spatial correlations between rice paddy extent and XCH4 are confounded by cross-correlation with other XCH4 emission sources that have similar spatial structures. As a result, the spatial and temporal consistencies between rice paddies and XCH4 reported in Zhang et al.1 do not imply a causal relationship. The inference of emissions based on the correlation may lead to incorrect conclusions on the annual variabilities of rice paddy CH4 emissions in Monsoon Asia.
The space-based instruments Greenhouse gases Observing SATellite Thermal And Near-infrared Sensor for carbon Observation—Fourier Transform Spectrometer (GOSAT TANSO-FTS) and SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY (SCIAMACHY) measure the column-averaged dry-air mole fraction of CH4, which is the ratio of vertical column densities (VCDs) between CH4 and dry air weighted by a column averaging kernel2,3. VCD is defined as the total number of molecules per unit area in a vertical column from the surface to the top of the atmosphere. The XCH4 observed from space is given by
in which \(f( \cdot )\) is the satellite measurement operator for averaging kernel convolution. Therefore, the variability of XCH4 is subjected to any possible changes of CH4 at different altitudes due to atmospheric transport, apart from the surface layer emissions. Previous studies have shown the significant impact of long-range transport on XCO2 variability4,5,6) and the same mechanism can be applied to XCH4. In the northern extratropics, the atmospheric zonal mixing time is estimated to be about 2 weeks7, which is much shorter than the seasonal cycle of CH4 fluxes. As a result, the seasonal variability of XCH4 observed at any specific location can be driven by the large scale advected signal instead of the local signal from the underlying surface methane flux. To quantify the relative contribution of a local and external signal, we conducted a tagged tracer simulation using the greenhouse gas framework-Flux (GHGF-Flux) forward model (see “Methods“ and Supplementary Fig. 1) for the four regions of interest (ROIs) in Zhang et al.1, including Northeast China, Southeast China, North Bangladesh, and North India, as shown in Fig. 1a. We can see that the external contribution to the seasonal cycle of XCH4 outweighs the local contribution for Northeast China, Southeast China, and North India, while they are comparable in North Bangladesh. To further investigate the drivers of XCH4 seasonal variability, Fig. 1b shows the monthly averaged XCH4 in the four ROIs and the corresponding zonal means of XCH4 over latitudinal bands centered on the ROIs. The local XCH4 seasonal variabilities are strongly correlated (p value < 0.01) with the zonal mean seasonal cycle in all four ROIs despite considerable scatter due to retrieval error and synoptic-scale XCH4 variability. Such agreement is expected since the seasonal cycle of XCH4 has previously been shown to have strong zonal features (Supplementary Fig. 2; ref. 3). These two pieces of evidence strongly suggest that the local variability in XCH4 has a much larger footprint than the underlying local region. Therefore, any causal argument for a correlation between XCH4 observations from space and local surface emissions needs to account the effect of long-range atmospheric transport.
Zhang et al.1 also claimed that the spatial distribution of rice paddies was a major factor in determining the spatial XCH4 distributions in monsoon Asia based on their spatial consistencies. However, there is also spatial consistency between XCH4 and the non-agriculture fluxes, and cross-correlation between agriculture and non-agriculture CH4 fluxes. From our analysis based on the emission database for global atmospheric research (EDGAR) reanalysis data as shown in Fig. 2a, the spatial correlation between non-agriculture CH4 emissions and XCH4 in Monsoon Asia is higher than that between agriculture and XCH4. It indicates the rice paddy emission may not be the most important factor regulating the spatial distribution of XCH4 in Monsoon Asia. Moreover, the non-agriculture and agriculture CH4 emissions are strongly cross-correlated in space (Fig. 2b) since agricultural lands in Monsoon Asia are usually close to the non-agriculture sources, which mainly include anthropogenic sources (energy and fossil fuel production) and waste and wastewater sources8. Such a strong cross-correlation should be accounted for when inferring a relationship between the spatial structure of XCH4 and agricultural flux, given that the non-agriculture sources in Asia are also highly variable in both space and time9.
Altogether, our re-analysis of the XCH4 observations combined with atmospheric transport model simulations suggests the need for caution in using correlation-based inference to quantify the change of paddy rice CH4 emissions from the simple relationship between the area and growth of paddy rice and satellite-observed XCH4. We suggest that combining satellite observations and model simulations in a data assimilation system (e.g., ref. 10) is needed to disentangle the influence of local rice paddy emissions from other sources within the region and large scale advected signals.
Methods
Datasets
The IMAP v7.2 XCH4 data product from SCIAMACHY retrievals, which were downloaded from the ESA GHG-CCI data portal (http://www.esa-ghg-cci.org/). The XCH4 data from 2003 to 2011 are used for analysis in this study. The EDGAR methane emission bottom-up inventory data are obtained from The Emissions Database for Global Atmospheric Research (EDGAR) (https://edgar.jrc.ec.europa.eu/overview.php?v=432_GHG). The annual sector-specific grid map in 2010 for total CH4 flux and for agriculture soil is used in this study.
Tagged Tracer simulations using GHGF-Flux simulation of CH4
Tagged tracer simulations were performed with the GHGF-Flux forward model. GHGF-Flux is a flux inversion system developed under NASA’s Carbon Monitoring System project. The GHGF is capable of simulating CH4, CO, CO2, and OCS and inherits the chemistry transport model from the GEOS-Chem. Chemical transport is driven by the Modern-Era Retrospective Analysis for Research and Applications, Version 2 (MERRA-2) meteorology produced with version 5.12.4 of the GEOS atmospheric data assimilation system11. To perform tracer transport, these fields are regridded to 2° × 2.5° horizontal resolution and archived with a temporal resolution of 3 h except for surface quantities and mixing depths, which have a temporal resolution of 1 h. Tracer transport is performed at 15 min time steps. Surface CH4 emissions were taken to be the total posterior CH4 flux from CarbonTracker-CH4 for 201010,12, regridded to the 2° × 2.5° model resolution. Global OH fields were obtained from the Global Modeling Initiative model simulation run with MERRA reanalysis. With these sources and sinks XCH4 is simulated over 2010–2015 (using repeated 2010 surface fluxes). Simulations are performed with surface fluxes at every model grid cell and local fluxes only for the four ROIs, from which the local and transported XCH4 signals are isolated. For the XCH4 simulation the ROIs are approximated as latitude-longitude boxes (see Supplementary Fig. 1). The North China box is bounded by 45°–59°N and 128.75°–136.25°E; North India is bounded by 25°–35°N, 68.75°–81.25°E; the North Bangledesh is bounded by 19°–25°N and 86.25°–93.75°E; and Southeast China is bounded by 25°–29°N and 113.75°–121.75°E. The 6-year XCH4 time series are then detrended and averaged across the 6 years to obtain a mean seasonal cycle (see Supplementary Fig. 5). Note that simulated XCH4 is calculated using a column averaging kernel with a value of 1 for every level.
Data availability
CarbonTracker-CH4 results are provided by NOAA ESRL, Boulder, Colorado, USA (http://www.esrl.noaa.gov/gmd/ccgg/carbontracker-ch4/); The IMAP v7.2 data product from SCIAMACHY from the ESA-CCI data portal (http://www.esa-ghg-cci.org/); the EDGAR methane emission bottom-up inventory data are provided by the European Commission (https://edgar.jrc.ec.europa.eu/overview.php?v=432_GHG). Results from model simulations are available via an open-access link at https://doi.org/10.5281/zenodo.4291324.
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Acknowledgements
Z.Z. would like to thank Yuk Yung at Caltech and Stan Sander at JPL for their strong supports and stimulating discussions on greenhouse gas remote sensing. BB’s research was supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Universities Space Research Association under contract with NASA. BB’s research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004).
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Z.Z. designed the study, conducted the analysis of satellite observations, and wrote the first draft. B.B. performed the model simulation and data analysis and wrote the draft. F.G. and Z.H. conducted the initial analysis of the original study by Zhang et al. L.L. interpreted the analysis of satellite observations. All co-authors collaborated in the interpretation of the results and editing of the paper.
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Zeng, ZC., Byrne, B., Gong, FY. et al. Correlation between paddy rice growth and satellite-observed methane column abundance does not imply causation. Nat Commun 12, 1163 (2021). https://doi.org/10.1038/s41467-021-21434-7
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DOI: https://doi.org/10.1038/s41467-021-21434-7
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