Literature DB >> 35410420

Global nature run data with realistic high-resolution carbon weather for the year of the Paris Agreement.

Anna Agustí-Panareda1, Joe McNorton2, Gianpaolo Balsamo2, Bianca C Baier3,4, Nicolas Bousserez2, Souhail Boussetta2, Dominik Brunner5, Frédéric Chevallier6, Margarita Choulga2, Michail Diamantakis2, Richard Engelen2, Johannes Flemming2, Claire Granier3,7,8, Marc Guevara9, Hugo Denier van der Gon10, Nellie Elguindi7, Jean-Matthieu Haussaire5, Martin Jung11, Greet Janssens-Maenhout12, Rigel Kivi13, Sébastien Massart2, Dario Papale14, Mark Parrington2, Miha Razinger2, Colm Sweeney4, Alex Vermeulen15, Sophia Walther11.   

Abstract

The CO2 Human Emissions project has generated realistic high-resolution 9 km global simulations for atmospheric carbon tracers referred to as nature runs to foster carbon-cycle research applications with current and planned satellite missions, as well as the surge of in situ observations. Realistic atmospheric CO2, CH4 and CO fields can provide a reference for assessing the impact of proposed designs of new satellites and in situ networks and to study atmospheric variability of the tracers modulated by the weather. The simulations spanning 2015 are based on the Copernicus Atmosphere Monitoring Service forecasts at the European Centre for Medium Range Weather Forecasts, with improvements in various model components and input data such as anthropogenic emissions, in preparation of a CO2 Monitoring and Verification Support system. The relative contribution of different emissions and natural fluxes towards observed atmospheric variability is diagnosed by additional tagged tracers in the simulations. The evaluation of such high-resolution model simulations can be used to identify model deficiencies and guide further model improvements.
© 2022. The Author(s).

Entities:  

Year:  2022        PMID: 35410420      PMCID: PMC9001646          DOI: 10.1038/s41597-022-01228-2

Source DB:  PubMed          Journal:  Sci Data        ISSN: 2052-4463            Impact factor:   8.501


Background & Summary

Reducing human-made emissions of CO2 is at the heart of the climate change mitigation efforts in the Paris Agreement. In support of such efforts, the CO2 Human Emission (CHE) project (www.che-project.eu) has designed a prototype system to monitor CO2 fossil fuel emissions at the global scale. This challenging task requires the capability to detect and quantify the localised and relatively small signals of fossil fuel emissions in the atmosphere compared to the large variability of background CO2 concentrations not directly affected by local sources, and to distinguish anthropogenic sources from vegetation fluxes[1-3]. Using observations of atmospheric constituents to estimate emissions[4,5] relies on a good understanding and accurate modelling of their atmospheric variability, which is largely determined by the weather-driven atmospheric transport together with surface biogenic fluxes and anthropogenic emissions. In the CHE project a library of nature runs of CO2 and species co-emitted with CO2 has been produced at different scales and with varying degrees of complexity[6] which complements previous nature runs[7]. Nature runs are very high-resolution simulations that mimic nature, in that they provide a realistic representation of processes of interest, in this case those modulating atmospheric CO2 variability. These simulations provide a reference for Observation System Simulation Experiments (OSSEs)[8] Quantitative Network Design (QND)[9]. In OSSEs and QND studies, synthetic observations extracted from nature runs are used to assess the impact of different observing system configurations[10]. It is envisaged that such a monitoring system will rely on the use of a large variety of measurements including species co-emitted with CO2 that can help to isolate the fossil fuel emissions[3,11]. The future CO2M (Copernicus CO2 Monitoring) satellite mission is purposely designed to provide a high-resolution imaging capability to detect CO2 emission hotspots with high-precision observations of atmospheric CO2 concentrations[2,3,12]. CO2M will complement a constellation of satellites[4] and a global in situ network[5] to quantify the atmospheric CO2 variability from which emissions will be derived with atmospheric inversion systems. Simulating a realistic distribution of CO2 and co-emitters depends on the representation of the surface fluxes, chemical sources/sinks, and atmospheric transport. Here we use the Copernicus Atmosphere Monitoring Service (CAMS) high-resolution forecast of CO2, CH4 and CO (https://atmosphere.copernicus.eu/charts/cams/carbon-dioxide-forecasts) which has been demonstrated to produce realistic and accurate variability of carbon weather[13-15]. The configuration of the nature run is shown in Fig. 1. Note that the CHE nature run is a free-running tracer simulation unlike the CAMS high-solution forecast which is initialised daily from an atmospheric composition analysis.
Fig. 1

(a) Schematic of production framework for CHE nature run dataset (details of different components of the simulation in the text); (b) Overview of CHE nature run model output and strategy for comparison with different types of observations of carbon tracers and other relevant datasets such as lower resolution simulations. The differences between the CHE nature run and the various observations can be used to estimate and shed light into the different sources of uncertainty (orange boxes).

(a) Schematic of production framework for CHE nature run dataset (details of different components of the simulation in the text); (b) Overview of CHE nature run model output and strategy for comparison with different types of observations of carbon tracers and other relevant datasets such as lower resolution simulations. The differences between the CHE nature run and the various observations can be used to estimate and shed light into the different sources of uncertainty (orange boxes). The CHE nature run aims to support scientific studies that will shed light on the challenges of estimating CO2 emissions with the goal to build a CO2 monitoring and verification support capacity[3]. These challenges span a wide range of aspects from sparse observing systems, consistency between ocean/land observations from different satellite-view modes[16], large variability in the biogenic signal[17], large representativity errors in anthropogenic emissions[13], transport errors[18] and stringent requirements of high accuracy observations to estimate small signal with respect to large background values[16,19]. This global high-resolution dataset can provide a reference for testing different approaches to address those challenges.

Methods

Modeling framework

The CAMS high resolution forecasting system at the European Centre for Medium Range Weather Forecasts (ECMWF)[13,14,20] has been used to produce the nature run dataset which includes simulations of CO2, CH4 and CO as illustrated in Fig. 1. It is based on the Integrated Forecasting System (IFS) model cycle 46R1 used to produce the operational weather forecast from June 2019 to June 2020[21]. The model has a reduced octahedral Gaussian grid[22] with a resolution of Tco1279 (corresponding to approximately 9 km) and 137 model levels. The simulations have been produced by running a sequence of 1-day IFS forecasts of the carbon tracers and weather. The weather forecasts are initialized with state-of-the-art re-analysis of meteorological fields (ERA5)[23]. The atmospheric tracers start from the CAMS re-analysis[24,25] initial conditions at the initial date of the dataset and from then onwards they are cycled from one forecast to the next in a free-running style. The different model components for the carbon weather forecast in the IFS, including the representation of the emissions for the different tracers, are listed in Table 1. All the emissions at the surface are prescribed except for the CO2 biogenic fluxes which are modelled online[26,27], providing consistency between the response of fluxes to atmospheric conditions and tracer transport[28]. There are various differences with respect to the CAMS operational high-resolution forecast in 2015: improved anthropogenic emissions[29-31] and natural CO2 ocean fluxes[32]; as well as an improved IFS model version[21] and initial conditions[23-25]. The configuration of the simulations with daily re-initialisation of the weather forecast and free-running tracers ensures consistency of the tracer evolution throughout the simulation by avoiding jumps in their concentrations brought by the assimilation of observations in the analysis, while maintaining a realistic and accurate simulation of their atmospheric transport and variability of the underlying biogenic fluxes from the model[26,27].
Table 1

Model components with emission datasets used as boundary conditions in the nature run simulation and prescribed atmospheric chemical sources/sinks.

Model components and emission datasetsSourceHorizontal and temporal resolutionReferences
Tracer advectionIFS semi-Lagrangian schemeModel resolution and time step[33,34,91,92]
Tracer convective transportIFS Tiedtke schemeModel resolution and time step[93,94]
tracer turbulent mixingIFS boundary layer schemeModel resolution and time step[9597]
CO2 biogenic fluxesIFS CTESSEL A-gs with bias correctionModel resolution and time step[26,27]
CO2 anthropogenic emissionsEDGARv4.5FT2015 annual emissions and EDGARv4.2FT2010 monthly scaling factors CAMS-GLOB-TEMPO daily scaling factors for residential heating, CAMS-GLOB-AIR monthly emissions from aviation0.1o × 0.1o, monthly, daily (residential sector)[2931]
CO2 ocean fluxesJena CarboScope v162.0o × 2.5o, daily fluxes averaged to monthly mean fluxes[32]
CO2, CH4, CO fire emissionsGFAS v1.20.1o × 0.1o, daily[63]
CH4 wetland fluxesLPJ-HYMN climatology (1990-2008)1o × 1o,monthly[98]
CH4 anthropogenic emissionsCAMS-GLOB-ANT v2.1 (based on EDGAR4.3.2 in 2012 and EDGARv4.2FT2010 seasonal cycle for 2010).0.1o × 0.1o, monthly[99,100]
CH4 other fluxesTermites, wild animals, ocean fluxes and soil sink1o × 1o,monthly[101104]
CO emissionsCAMS-GLOB-ANT v2.10.1o × 0.1o, monthly[99,100]
CO chemistryLinear CO chemistry schemeModel resolution and time step[105]
CH4 chemical loss rateClimatological loss rate6o × 4o, monthly[106]

Model resolution is around 9 km and model time step is 7.5 minutes.

Model components with emission datasets used as boundary conditions in the nature run simulation and prescribed atmospheric chemical sources/sinks. Model resolution is around 9 km and model time step is 7.5 minutes.

Model output

The standard parameters available from the CHE nature run dataset are listed in Table 2 and Table S1 in Supplementary Information file 1. Additional experimental tagged tracers are provided to characterize the atmospheric enhancement associated with the natural surface fluxes and anthropogenic emissions (Table 3). The enhancement can be computed by subtracting the concentrations of the background tracer without the specific emission/flux from the tracer concentration with the flux/emission. This assumes that the transport is linear. It is worth noting that artificial negative enhancements can occur in the vicinity of plumes due to numerical oscillations associated with the cubic interpolation of the advection scheme around very steep gradients. This can be considered a numerical error in the simulation. The CO2 tagged tracers are simulated without applying any mass fixer in order to ensure the signal comes only from the flux. The tagged tracers provide the enhancement during each 1-day simulation as they are re-initialised every day at 00UTC in order to avoid growing errors associated with the mass conservation[33,34]. This means the flux enhancement is reset to zero at 00 UTC. Detailed information on those tracers is provided in Table 4.
Table 2

Content of CHE nature run dataset with different parameter types and their associated data volume for the full year.

Parameters types and levelsArchived time stepRange of data volume
per parameter in GBytes
Model levels parameters from level 1 (model top) to level 137 (model bottom)*3-hourly9–7,373
Pressure level parameters: 1, 2, 3, 5, 7, 10, 20, 30, 50, 70, 100 to 300 by 50, 400 to 700 by 100, 850, 925, 950, 1000 hPa3-hourly219–1,241
Parameters on surface layers3-hourly~146
1: 0–7 cm, 2: 7–21 cm, 3: 21–72 cm, 4: 72 cm–1.82 m
2D surface fields3-hourly~55
2D prescribed daily emissionsdaily~7
2D prescribed monthly emissionsmonthly~0.24
3D prescribed monthly aviation emissions on model levels from level 1 (model top) to level 137 (model bottom)monthly~33

*Model levels can be converted to pressure levels p with the following equation pi = psfcBi + Ai [in Pa] where psfc is surface pressure and Ai and Bi are static coefficients defined for each model level i (https://confluence.ecmwf.int/display/UDOC/L137 + model + level + definitions). The volume of atmospheric-tracer parameters has been highlighted in bold. The individual parameters are listed in Supplementary Information file 1 (Table S1).

Table 3

List of experimental CO2 tagged tracers from the CHE nature run dataset.

Tagged tracersParameter typeParameter IDUnitsEnhancement processing (parameter IDs)
CO2 tracer3D (model and pressure levels)12.212kg kg-1
CO2 tracer without fire emissions3D (model and pressure levels)13.212kg kg−13D Biomass burning (12.212-13.212)
CO2 tracer without anthropogenic emissions3D (model and pressure levels)14.212kg kg−13D Anthropogenic (12.212-14.212)
CO2 tracer without biogenic fluxes3D (model and pressure levels)15.212kg kg−13D Biogenic (12.212-15.212)
CO2 tracer without ocean fluxes3D (model and pressure levels)16.212kg kg−13D Ocean (12.212-16.212)
Total-column CO2 tracer2D (surface level)112.212kg m−2
Total-column CO2 tracer without fire emissions2D (surface level)113.212kg m−2Column Biomass burning (112.212-113.212)***
Total-column CO2 tracer without anthropogenic emissions2D (surface level)114.212kg m−2Column Anthropogenic (112.212-114.212)***
Total-column CO2 tracer without biogenic emissions2D (surface level)115.212kg m−2Column Biogenic (112.212-115.212)***
Total-column CO2 tracer without ocean fluxes2D (surface level)116.212kg m−2Column Ocean (112.212-116.212)***

Each tracer is identified with a given experimental parameter ID. ***Note that the units of tagged tracers for the total column need to be converted from kg m−2 to ppm as described in 2D Atmospheric Composition parameters.

Table 4

Distribution of XCO2 anthropogenic enhancement (XCO2_FF) accumulated over a 24-hour period from the CHE global nature run as mean number (and percentage in bold) of model cells with XCO2_FF > 0.25 ppm (left columns) and XCO2_FF > 0.50ppm (right columns).

XCO2_FF > 0.25 ppm Number model cells % model cells (Number clear-sky model cells) (% clear-sky model cells)XCO2_FF > 0.50 ppm Number model cells % model cells (Number clear-sky model cells) (% clear-sky model cells)
LandCoastOceanLandCoastOcean
January36,533 + /−2,45841,018 + /−192415,689 + /−3,03114,933 + /−1,31218,178 + /−1,2435,444 + /−1475
0.55 + /−0.040.62 + /−0.030.24 + /−0.050.23 + /−0.020.28 + /−0.020.08 + /−0.02
(11,194 + /−2,468)(10,809 + /−3,101)(3745 + /−1,466)(4,995 + /−1,599)(5,096 + /−1,915)(1,471 + /−853)
(0.17 + /−0.04)(0.16 + /−0.05)(0.06 + /−0.02)(0.08 + /−0.02)(0.08 + /−0.03)(0.02 + /−0.01)
July24,352 + /−1,23528,203 + /−8679,107 + /−22128,603 + /−58311,325 + /−6102,901 + /−954
0.37 + /−0.020.43 + /−0.010.14 + /−0.030.13 + /−0.010.17 + /−0.010.04 + /−0.01
(6,314 + /−1,288)(5,746 + /−1,556)(2,181 + /−1169)(2,238 + /−613)(2,289 + /−768)(732 + /−554)
(0.10 + /−0.02)(0.09 + /−0.02)(0.03 + /−0.02)(0.03 + /−0.01)(0.03 + /−0.01)(0.01 + /−0.01)

The variability with respect to the mean number is shown by the +/− standard deviation. The statistics are also provided for clear-sky conditions, land, ocean and coastal regions, as these considerations are all relevant for satellite observations. Clear-sky model cells are defined with a cloud fraction threshold less than 10% over the 9 km × 9 km model cell; land cells have more than 99% land; ocean cells have less than 1% land and model cells over the coast have land between 1 and 99%.

Content of CHE nature run dataset with different parameter types and their associated data volume for the full year. *Model levels can be converted to pressure levels p with the following equation pi = psfcBi + Ai [in Pa] where psfc is surface pressure and Ai and Bi are static coefficients defined for each model level i (https://confluence.ecmwf.int/display/UDOC/L137 + model + level + definitions). The volume of atmospheric-tracer parameters has been highlighted in bold. The individual parameters are listed in Supplementary Information file 1 (Table S1). List of experimental CO2 tagged tracers from the CHE nature run dataset. Each tracer is identified with a given experimental parameter ID. ***Note that the units of tagged tracers for the total column need to be converted from kg m−2 to ppm as described in 2D Atmospheric Composition parameters. Distribution of XCO2 anthropogenic enhancement (XCO2_FF) accumulated over a 24-hour period from the CHE global nature run as mean number (and percentage in bold) of model cells with XCO2_FF > 0.25 ppm (left columns) and XCO2_FF > 0.50ppm (right columns). The variability with respect to the mean number is shown by the +/− standard deviation. The statistics are also provided for clear-sky conditions, land, ocean and coastal regions, as these considerations are all relevant for satellite observations. Clear-sky model cells are defined with a cloud fraction threshold less than 10% over the 9 km × 9 km model cell; land cells have more than 99% land; ocean cells have less than 1% land and model cells over the coast have land between 1 and 99%. Figure 1b provides an overview of the different types of model output from the CHE nature run dataset and how these can be compared to other datasets including various types of observations[5,35,36] as well as atmospheric inversions/simulations of carbon tracers[9]. Such a comparison can shed some light on the different components of the uncertainty in the simulations of carbon tracers coming from the surface fluxes, the atmospheric transport and the representativity error associated with the limited model resolution[14]. A complementary lower resolution ensemble of simulations[18] (25 km in the horizontal) has been also produced using the same model setup which provides information on emission uncertainty[30], transport uncertainty and impact of meteorological uncertainty on biogenic fluxes. Two other major sources of uncertainty stem from the initial conditions of the carbon tracers at the beginning of the simulation[24,25] and the biogenic flux model[26,27]. An estimation of these uncertainties is provided in the Technical Validation section.

Example: Using tagged tracers to characterise anthropogenic plumes over land and ocean

In order to monitor anthropogenic CO2 emissions, it is crucial to observe the CO2 plumes emanating from the emission sources. These observations need to be based either targeted field campaign observations[13] or on high resolution imaging satellites[10]. As satellites have different viewing geometries over land and ocean[16], it is very important to understand how many of these plumes are located over land, ocean and coastal regions. Moreover, satellite observations only provide total column CO2 over cloud-free regions. Table 4 provides an example of statistics on the proportion of anthropogenic plumes accumulated over a 24-hour period over land/ocean and the proportion of plumes under cloudy conditions for January and July 2015. These fossil fuel tagged tracers and other tagged tracers associated with the biogenic fluxes, ocean fluxes and biomass burning emissions are all included in the CHE nature run dataset (see Table 3).

Example: Insights into total column variability

The CO2, CH4 and CO observing system is based on in situ observations, at the surface or from tall towers, and remote sensing observations from ground-based stations or satellites providing partial/total column observations. There are currently very few vertical profile observations from aircrafts[37,38] and Aircore measurements[36,39] that can be used to link the two observation types. For low-resolution transport models assimilating both surface and total column observations in an atmospheric inversions framework, it can sometimes be challenging to combine the surface and total column variability for various reasons. These include errors in the remote sensing observations[16], representation errors near the surface and model transport errors associated with vertical mixing[40], atmospheric chemistry[41], as well as long-range transport[42] and the impact of stratospheric intrusions[43]. The global nature run can be useful to characterize the column variability of carbon tracers[44] associated with transport. Figure 2 illustrates the potential use of the CHE nature run to explain the variability of XCO2, XCH4 and XCO at 24 TCCON sites (https://tccondata.org). The coefficient of determination shows that the variance of the total column can be explained by the different layers in the column in the nature run. When the column is well mixed, the contribution from the different layers is similar. At the sites where the influence of local emissions or natural fluxes is strong, the layers near the surface dominate the variability. Long-range transport in the free troposphere and upper troposphere/lower stratosphere also plays an important role, as depicted by the green/orange bars with higher r2 values than the near-surface layers in purple/red. The dataset can also be used to assess the important contribution of the stratosphere in the variability of XCH4[45].
Fig. 2

Coefficient of determination (r2) [%] of CO2, CH4 and CO total column with different partial layers in the atmospheric column in January and July 2015 at 24 TCCON sites (tccon.org). The atmospheric layers are defined as follows: from surface to 400 m (SFC), from 400 to 2 km (BL), from 2 km to 5 km (FT), from 5 km to 10 km (UTLS), from 10 km to the top of atmosphere (STRAT). All the column and partial column data have been detrended before calculating the coefficient of determination. All r2 values shown are statistically significant with p-value < 0.01 except when the r2 < 0.001.

Coefficient of determination (r2) [%] of CO2, CH4 and CO total column with different partial layers in the atmospheric column in January and July 2015 at 24 TCCON sites (tccon.org). The atmospheric layers are defined as follows: from surface to 400 m (SFC), from 400 to 2 km (BL), from 2 km to 5 km (FT), from 5 km to 10 km (UTLS), from 10 km to the top of atmosphere (STRAT). All the column and partial column data have been detrended before calculating the coefficient of determination. All r2 values shown are statistically significant with p-value < 0.01 except when the r2 < 0.001.

Data Records

The CHE nature run dataset can be accessed through the ECMWF API following the examples provided in[46]. The data can be extracted on the native octahedral grid with the original resolution (tco1279, corresponding to approximately 9 km) or on a regular latitude/longitude grid at the required resolution of the user. Both grib and NetCDF formats are available. The dataset extends from 26 December 2014 to 31 December 2015. The list of contents is provided in Table 2. All meteorological and tracer fields and surface fluxes have been archived with 3-hourly time steps with respect to the 00 UTC initialization of the weather forecast. Step 0 of all the meteorological parameters represents the initial conditions taken from ERA5[23]. Atmospheric species (CO2, CH4 and CO) at step 0 are equivalent to tracers from the previous day at step 24, because they are free-running from one 1-day forecast to the next as illustrated in Fig. 1. Note that the emissions of CO and the CO2 emissions from aviation are not stored in the CHE nature run dataset, but they can be obtained from the Copernicus Atmosphere Data Store (https://ads.atmosphere.copernicus.eu).

Technical Validation

The dataset is based on the state-of-the-art operational NWP and CAMS forecasting system[21,47] which has been proven to produce reliable and accurate atmospheric CO2, CH4 and CO variability[13-15]. The CHE nature run focuses on 2015, a year characterised by a pronounced decrease in the terrestrial carbon sink associated with the strong El Niño Southern Oscillation (ENSO) of 2015-2016[48] with droughts[49], as well as fires in several regions, particularly over the tropics[50]. The larger than normal CO2 atmospheric growth rate in 2015[48,51] and anomalously high fire emissions are well captured by the CHE nature run with a total global annual flux of 6.60 GtC (equivalent to 3.16 ppm/year from 1 January 2015 to 31 December 2015), which is close to the NOAA estimate of 2.99 + /−0.07 ppm/year (https://www.esrl.noaa.gov/gmd/ccgg/trends/global.html). The CO2 components of the budget include 9.29 GtC of anthropogenic emissions, 2.09 GtC of fire emissions, 2.10 GtC ocean sink and 2.69 GtC sink from land ecosystems. These values are consistent with the global carbon budget estimates[52].

Example: Evaluation of CO2 sources/sink by vegetation

Biogenic CO2 fluxes associated with vegetation over land can dominate atmospheric CO2 variability on a wide range of time scales from diurnal, synoptic, seasonal to inter-annual[28]. They are a crucial component for the estimation of the background CO2 underlying the fossil fuel plumes from emission hotspots. This background CO2 has not been directly influenced by the plumes emanating from local anthropogenic sources, but it results from the larger-scale fluxes associated with biogenic sources and sinks over land. The European Eddy Covariance (EC) ecosystem flux data collected and processed by the Integrated Carbon Observation System (ICOS)[53] are used to evaluate the uncertainty of modelled biogenic fluxes in the IFS (Fig. 3) which are bias-corrected[27] in the CHE nature run. These modelled fluxes are also compared to other flux products, such as FLUXCOM[54,55] (extended to include varying diurnal meteorology from ERA5) and the CAMS CO2 inversion (v18r3) product[56,57]. The EC data were processed and the Gross Primary Production (GPP) and ecosystem respiration (Reco) estimated using the standard methods applied in FLUXNET[58] using the observed Net Ecosystem Exchange (NEE). Fig. 3 shows an overall underestimation of the seasonal cycle of NEE, GPP and Reco at the EC sites with typical errors of around 2 μmol m−2 s−1. Synoptic-scale errors are smaller while the diurnal cycle has larger errors of around 4 μmol m−2 s−1 (not shown in Fig. 3). This underestimation is exacerbated by the anomalously high NEE and Reco observed during the European drought in 2015 (Fig. SB7.3[49]). This type of evaluation can be used to understand the source of biogenic flux errors and improve the underlying biogenic models, as well as to quantify the uncertainty of prior fluxes for atmospheric inversions[59].
Fig. 3

Mean seasonal cycle of CO2 biogenic fluxes [μmol m−2 s−1] at the 25 Eddy Covariance sites. FLUXNET2015[58] observations [ICOS 2018 drought dataset[53]] are shown in black; the IFS modelled fluxes in cyan and the bias corrected fluxes used in the CHE nature run in blue; the CAMS inversion product[56,57,65] (total flux –anthropogenic emissions) based on surface observations is shown in orange; and the CHE FLUXCOM product[54,55] in green. The shading depicts the standard deviation across the 25 sites.

Mean seasonal cycle of CO2 biogenic fluxes [μmol m−2 s−1] at the 25 Eddy Covariance sites. FLUXNET2015[58] observations [ICOS 2018 drought dataset[53]] are shown in black; the IFS modelled fluxes in cyan and the bias corrected fluxes used in the CHE nature run in blue; the CAMS inversion product[56,57,65] (total flux –anthropogenic emissions) based on surface observations is shown in orange; and the CHE FLUXCOM product[54,55] in green. The shading depicts the standard deviation across the 25 sites.

Example: Simulation and observation mismatch in the total column of CO2, CH4 and CO

The TCCON data[60] which is widely used as a reference to evaluate biases in global measurement of CO2, CH4 and CO total column averages–referred to as XCO2, XCH4 and XCO–from space[16] is used here to assess the inter-hemispheric gradient, seasonal cycle and synoptic day-to-day variability in the nature run dataset (Fig. 4). The large-scale patterns of variability on a monthly scale are generally well represented for the three species. The amplitude of the XCO2 seasonal cycle is underestimated at most TCCON sites, with the summer trough being 1 to 3 ppm higher than observed. This is consistent with the general underestimation of the biogenic sink during the growing season shown in Fig. 3. XCH4 is overestimated in spring/summer and underestimated in autumn/winter, due to errors in the seasonality of the chemical sink and emissions (e.g. wetlands, agriculture and biomass burning). XCO is underestimated in winter which is a common feature in many models and emission data sets[61] and overestimated in summer/autumn, often caused by the biogenic emissions of isoprene, which have a large impact on southern hemisphere and global background values[62] of CO. Other sources of error are associated with the chemical sources/sinks[61] and fire emissions[63], as 2015 was an extreme year for CO because of Indonesian fires in autumn[64]. Part of the bias shown in Fig. 4 also comes from the CO2, CH4 and CO initial conditions at the start of the nature run extracted from the CAMS re-analysis[24,25]. The random error in the sub-monthly variability (STDE in Fig. 4) - associated with surface fluxes/emissions and atmospheric transport - is generally below 1.5 ppm for XCO2, 10 ppb for XCH4 and 10 ppb for XCO, except at urban sites near emission hotspots such as Pasadena, Tsukuba and Paris.
Fig. 4

Evaluation of XCO2, XCH4 and XCO from the CHE nature run (NR). The nature run is compared to total column FTIR observation[35,60] at the TCCON stations[67–90] (OBS). The crosses indicate that the bias is statistically significant (p-value < 0.01).

Evaluation of XCO2, XCH4 and XCO from the CHE nature run (NR). The nature run is compared to total column FTIR observation[35,60] at the TCCON stations[67-90] (OBS). The crosses indicate that the bias is statistically significant (p-value < 0.01).

Example: Fine-scale structure in vertical profiles

The vertical profiles of CO2, CH4 and CO are illustrated in Fig. 5 with a comparison to AirCore observations[36,39] from the National Oceanic and Atmospheric Administration (NOAA) Global Monitoring Laboratory and the lower-resolution CAMS surface in situ inversion dataset[57,65,66]. While most global transport models used in atmospheric inversion systems have too coarse horizontal and vertical resolution to be able to represent the fine-scale vertical structure, the CHE nature run is able to capture the small-scale anomalies along the atmospheric column from the surface up to the lower stratosphere (50 hPa). The profiles on three different consecutive days show the large variability associated with day-to-day synoptic transport, particularly for CO2. Capturing this type of vertical variability is important because it reflects the ability of atmospheric transport models to represent vertical mixing and long-range transport. Both need to be accurately represented in atmospheric inversions in order to accurately infer surface fluxes. Examples of anticorrelation between the near-surface CO2 and XCO2 are also shown in Fig. 5j (e.g. 7, 9, 15, 20, 21 and 24 June) which are associated with the advection of anomalously high/low CO2 air in the free troposphere (above 700 hPa) and the opposite decrease/increase of CO2 near the surface. This emphasizes the importance of tracer transport above the planetary boundary layer in explaining the variability of XCO2 also shown in Fig. 2.
Fig. 5

Examples of CO2 CH4 and CO vertical profiles from the CHE nature run at Sodankylä (67.37°N, 26.63°E). The nature run is compared to NOAA AirCore (v20201223) observations[36,39] and the CAMS CO2 and CH4 inversion[57,65,66] (a–i) during three days in June, depicted by the dashed lines in (j) where the nature run hovmöller plot for CO2 shows the temporal variability of the vertical profile at Sodankylä over the whole month of June. The solid black and magenta lines show the time series of XCO2 and near-surface CO2 averaged over the model levels from the surface to 400 m above the surface (SFC CO2) respectively.

Examples of CO2 CH4 and CO vertical profiles from the CHE nature run at Sodankylä (67.37°N, 26.63°E). The nature run is compared to NOAA AirCore (v20201223) observations[36,39] and the CAMS CO2 and CH4 inversion[57,65,66] (a–i) during three days in June, depicted by the dashed lines in (j) where the nature run hovmöller plot for CO2 shows the temporal variability of the vertical profile at Sodankylä over the whole month of June. The solid black and magenta lines show the time series of XCO2 and near-surface CO2 averaged over the model levels from the surface to 400 m above the surface (SFC CO2) respectively. Supplementary Information file 1
Measurement(s)atmospheric carbon dioxide, methane and carbon monoxide
Technology Type(s)numerical simulation
Factor Type(s)None
Sample Characteristic - Organismlong-lived greenhouse gases
Sample Characteristic - Environmentatmosphere
Sample Characteristic - Locationglobal atmosphere
  5 in total

1.  Role of atmospheric oxidation in recent methane growth.

Authors:  Matthew Rigby; Stephen A Montzka; Ronald G Prinn; James W C White; Dickon Young; Simon O'Doherty; Mark F Lunt; Anita L Ganesan; Alistair J Manning; Peter G Simmonds; Peter K Salameh; Christina M Harth; Jens Mühle; Ray F Weiss; Paul J Fraser; L Paul Steele; Paul B Krummel; Archie McCulloch; Sunyoung Park
Journal:  Proc Natl Acad Sci U S A       Date:  2017-04-17       Impact factor: 11.205

2.  Fire carbon emissions over maritime southeast Asia in 2015 largest since 1997.

Authors:  V Huijnen; M J Wooster; J W Kaiser; D L A Gaveau; J Flemming; M Parrington; A Inness; D Murdiyarso; B Main; M van Weele
Journal:  Sci Rep       Date:  2016-05-31       Impact factor: 4.379

3.  Statistical characterization of urban CO2 emission signals observed by commercial airliner measurements.

Authors:  Taku Umezawa; Hidekazu Matsueda; Tomohiro Oda; Kaz Higuchi; Yousuke Sawa; Toshinobu Machida; Yosuke Niwa; Shamil Maksyutov
Journal:  Sci Rep       Date:  2020-05-14       Impact factor: 4.379

4.  The Orbiting Carbon Observatory (OCO-2) tracks 2-3 peta-gram increase in carbon release to the atmosphere during the 2014-2016 El Niño.

Authors:  Prabir K Patra; David Crisp; Johannes W Kaiser; Debra Wunch; Tazu Saeki; Kazuhito Ichii; Takashi Sekiya; Paul O Wennberg; Dietrich G Feist; David F Pollard; David W T Griffith; Voltaire A Velazco; M De Maziere; Mahesh K Sha; Coleen Roehl; Abhishek Chatterjee; Kentaro Ishijima
Journal:  Sci Rep       Date:  2017-10-19       Impact factor: 4.379

  5 in total

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