EM-Earth: The Ensemble Meteorological Dataset for Planet Earth

Guoqiang Tang University of Saskatchewan, Canmore, Alberta, Canada;

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Martyn P. Clark Centre for Hydrology, University of Saskatchewan, Canmore, Alberta, and Department of Geography and Planning, University of Saskatchewan, Saskatoon, Saskatchewan, Canada;

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Simon Michael Papalexiou Department of Civil Engineering, University of Calgary, Alberta, and Department of Civil, Geological and Environmental Engineering, University of Saskatchewan, Saskatoon, Saskatchewan, Canada

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Abstract

Gridded meteorological estimates are essential for many applications. Most existing meteorological datasets are deterministic and have limitations in representing the inherent uncertainties from both the data and methodology used to create gridded products. We develop the Ensemble Meteorological Dataset for Planet Earth (EM-Earth) for precipitation, mean daily temperature, daily temperature range, and dewpoint temperature at 0.1° spatial resolution over global land areas from 1950 to 2019. EM-Earth provides hourly/daily deterministic estimates, and daily probabilistic estimates (25 ensemble members), to meet the diverse requirements of hydrometeorological applications. To produce EM-Earth, we first developed a station-based Serially Complete Earth (SC-Earth) dataset, which removes the temporal discontinuities in raw station observations. Then, we optimally merged SC-Earth station data and ERA5 estimates to generate EM-Earth deterministic estimates and their uncertainties. The EM-Earth ensemble members are produced by sampling from parametric probability distributions using spatiotemporally correlated random fields. The EM-Earth dataset is evaluated by leave-one-out validation, using independent evaluation stations, and comparing it with many widely used datasets. The results show that EM-Earth is better in Europe, North America, and Oceania than in Africa, Asia, and South America, mainly due to differences in the available stations and differences in climate conditions. Probabilistic spatial meteorological datasets are particularly valuable in regions with large meteorological uncertainties, where almost all existing deterministic datasets face great challenges in obtaining accurate estimates.

© 2022 American Meteorological Society. For information regarding reuse of this content and general copyright information, consult the AMS Copyright Policy (www.ametsoc.org/PUBSReuseLicenses).

Corresponding author: Guoqiang Tang, guoqiang.tang@usask.ca

Abstract

Gridded meteorological estimates are essential for many applications. Most existing meteorological datasets are deterministic and have limitations in representing the inherent uncertainties from both the data and methodology used to create gridded products. We develop the Ensemble Meteorological Dataset for Planet Earth (EM-Earth) for precipitation, mean daily temperature, daily temperature range, and dewpoint temperature at 0.1° spatial resolution over global land areas from 1950 to 2019. EM-Earth provides hourly/daily deterministic estimates, and daily probabilistic estimates (25 ensemble members), to meet the diverse requirements of hydrometeorological applications. To produce EM-Earth, we first developed a station-based Serially Complete Earth (SC-Earth) dataset, which removes the temporal discontinuities in raw station observations. Then, we optimally merged SC-Earth station data and ERA5 estimates to generate EM-Earth deterministic estimates and their uncertainties. The EM-Earth ensemble members are produced by sampling from parametric probability distributions using spatiotemporally correlated random fields. The EM-Earth dataset is evaluated by leave-one-out validation, using independent evaluation stations, and comparing it with many widely used datasets. The results show that EM-Earth is better in Europe, North America, and Oceania than in Africa, Asia, and South America, mainly due to differences in the available stations and differences in climate conditions. Probabilistic spatial meteorological datasets are particularly valuable in regions with large meteorological uncertainties, where almost all existing deterministic datasets face great challenges in obtaining accurate estimates.

© 2022 American Meteorological Society. For information regarding reuse of this content and general copyright information, consult the AMS Copyright Policy (www.ametsoc.org/PUBSReuseLicenses).

Corresponding author: Guoqiang Tang, guoqiang.tang@usask.ca

Meteorological data are fundamental to understanding global water and energy cycles (Trenberth et al. 2007, 2009; Schneider et al. 2013; L’Ecuyer et al. 2015; Rodell et al. 2015). A variety of geoscientific and operational applications, such as hydrological modeling and climate studies, need gridded meteorological inputs of variables such as precipitation, temperature, and humidity (Clark et al. 2015a,b; Hamman et al. 2018; Nguyen et al. 2018).

Many gridded meteorological datasets have been developed with different spatiotemporal coverage and resolution, different meteorological variables, different application objectives, and different data sources (Maggioni et al. 2016; Sun et al. 2018). Ground stations are the most important data source used to produce and validate gridded meteorological datasets (Sheffield et al. 2006; Livneh et al. 2015; Fick and Hijmans 2017; Tang et al. 2020b; Harris et al. 2020) given their high accuracy and long temporal coverage in many station networks (Menne et al. 2012). However, station networks have disadvantages such as limited spatial coverage in remote/undeveloped regions and temporal discontinuities caused by missing records and incomplete observation periods (Eischeid et al. 2000; Kidd et al. 2017; Tang et al. 2020a). Remote sensing techniques and numerical weather prediction models provide additional information to produce gridded meteorological datasets with global coverage at high spatiotemporal resolutions (Sorooshian et al. 2000; Huffman et al. 2007; Hou et al. 2014; Gelaro et al. 2017; Hersbach et al. 2020). Most remote sensing and model datasets rely on station observations for bias correction, data assimilation, and quality validation (Adler et al. 2003; Ashouri et al. 2015; Ma et al. 2018; Beck et al. 2019).

Existing meteorological datasets are typically deterministic, providing a single estimate of a given meteorological variable for a specific location and time step. Stations suffer from point-to-area interpolation uncertainties and measurement errors such as precipitation evaporation/wetting loss and undercatch/overcatch (Goodison et al. 1998; Yang et al. 2005; Scaff et al. 2015; Kochendorfer et al. 2018). Remote sensing techniques face challenges of imperfect retrieval algorithms, instrument limitations, insufficient sampling, and signal attenuation (Dinku et al. 2002; Adler et al. 2017; Beck et al. 2017; Tang et al. 2020b). Numerical weather prediction models are limited by imperfect model representations of physical processes and observational constraints (Donat et al. 2014; Parker 2016). Applications based on deterministic datasets may ignore these uncertainties. This is particularly true for remote regions and complex climatic/topographic conditions where almost all meteorological datasets exhibit large uncertainties due to sparse/unreliable measurements and imperfect models/algorithms (Gao et al. 2012; Henn et al. 2018; Newman et al. 2020).

Probabilistic datasets have advantages in estimating uncertainties and representing extremes (Kirstetter et al. 2015; Mendoza et al. 2017; Frei and Isotta 2019). Yet probabilistic datasets often have large data size, may be difficult to interpret, and their applications require more computational resources. Currently, a few datasets provide explicit uncertainty estimates, such probabilistic datasets include the HadCRUT4 global temperature dataset with 100 members (Morice et al. 2012), the Spatially Coherent Probabilistic Extended Climate dataset (SCOPE Climate) with 25 members in France (Caillouet et al. 2019), the ensemble precipitation and temperature datasets with 100 members in the United States and parts of Canada (Newman et al. 2015, 2019, 2020), and the Ensemble Meteorological Dataset for North America (EMDNA) with 100 members (Tang et al. 2021). Recently, several deterministic datasets offer probabilistic realizations, such as the ensemble version (Cornes et al. 2018) of the Europe-wide E-OBS temperature and precipitation dataset (Haylock et al. 2008), and the High-Resolution Ensemble Precipitation Analysis (Khedhaouiria et al. 2020) as the ensemble version of the Canadian Precipitation Analysis (CaPA; Mahfouf et al. 2007; Fortin et al. 2015). However, a global probabilistic meteorological dataset has not yet been developed.

Here we develop the Ensemble Meteorological Dataset for Planet Earth (EM-Earth) dataset, which provides estimates of precipitation, mean daily temperature (Tmean), daily temperature range (Trange), and dewpoint temperature (Tdew) at 0.1° resolution from 1950 to 2019 for global land areas. Precipitation, Tmean, and Tdew estimates are also available at the hourly scale. EM-Earth utilizes station data from the Serially Complete Earth (SC-Earth) dataset developed by Tang et al. (2021a), a global station dataset without temporal discontinuities. SC-Earth is merged with ERA5 to generate global gridded meteorological estimates and uncertainties. To meet the requirement of diverse applications, EM-Earth provides two types of datasets: the daily and hourly deterministic dataset, and the daily probabilistic dataset with 25 members (Fig. 1).

Fig. 1.
Fig. 1.

Flowchart demonstrating the production of EM-Earth deterministic and probabilistic estimates.

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

Datasets

Datasets used in this study (summarized in Table 1) can be divided into input sources, auxiliary data, validation stations, and intercomparison datasets.

Table 1.

Datasets used in the production and validation of EM-Earth.

Table 1.

Input data.

The two major inputs of EM-Earth are the SC-Earth and ERA5. SC-Earth was developed to address the temporal discontinuities of station measurements caused by occasional/seasonal missing records, values failed in quality control, and incomplete observation periods (Eischeid et al. 2000; Feng et al. 2004; Wang et al. 2017). Gap filling of station data can improve the quality of gridded meteorological estimates according to Longman et al. (2020) in Hawaii and Tang et al. (2021b) in North America. To illustrate this point, Tang et al. (2021b) compared the performance of raw station observations and a gap-filled dataset in gridded precipitation and temperature estimation over North America from 1979 to 2018 using various interpolation methods. They showed that gap filling improves the accuracy and trend of gridded estimates, with improvements due to gap filling more notable for lower station densities.

SC-Earth uses station data from the Global Historical Climatology Network Daily (GHCN-D; Menne et al. 2012) and the Global Surface Summary of the Day (GSOD; https://data.gov/index.html). Raw station observations have undergone strict quality control, and only stations with at least 8-yr records were used (Tang et al. 2021a). Tmean and Trange were calculated, respectively, as the mean of and difference between daily maximum and minimum air temperature from station data. That is desirable as some stations only provide Tmean data, and also, constraining Trange to be positive is easier than constraining the maximum temperature to be larger than the minimum; the potential skewness of diurnal temperature cycle was not considered. SC-Earth imputes missing values using 15 strategies based on four methods including quantile mapping, spatial interpolation/regression, machine learning, and multisource merging. A climatological correction based on quantile mapping and quantile delta mapping is applied to further improve the SC-Earth estimates. SC-Earth includes 64,399, 35,925, 34,851, 12,310, and 12,872 stations for precipitation, Tmean, Trange, Tdew, and wind speed, respectively. The station density of SC-Earth is constant from 1950 to 2019 and higher than many raw station datasets. For example, GHCN-D has ∼113,000 precipitation stations in total, while 90% of years before 2020 have fewer than 40,000 stations. Wind speed is not a target variable of EM-Earth because of the potential inhomogeneities in raw station data (Tang et al. 2021a). The average fractions of filled data are ∼55% for precipitation, Tmean, and Trange, and ∼59% for Tdew. The fractions are higher in early years due to sparse station networks.

ERA5 provides hourly near-surface estimates of precipitation, minimum temperature, maximum temperature, and Tdew. Tmean and Trange are inferred from minimum and maximum temperatures. We use ERA5 because it is the reanalysis product with the highest spatial and temporal resolution during 1950–2019, and its estimates can complement SC-Earth station data in sparsely gauged regions. In addition, ERA5 air temperature estimates at different pressure levels are used as auxiliary data to calculate near-surface temperature lapse rate to support spatial downscaling of ERA5 near-surface Tmean estimates. ERA5 ensemble estimates are not used because the Ensemble Data Assimilation (EDA) of ERA5 has coarse spatial resolution and incomplete uncertainty representation. Instead, EM-Earth uncertainties are estimated directly by using station data for cross validation. Other reanalysis products are not used because their spatiotemporal resolutions and temporal coverage do not meet the requirement of this study.

Auxiliary datasets.

Elevation data are from the Multi-Error-Removed Improved-Terrain (MERIT) digital elevation model (DEM) at 3″ (∼90 m at the equator) resolution (Yamazaki et al. 2017). MERIT DEM is spatially averaged to the 0.1° resolution to provide auxiliary information for spatial interpolation of station data. The MERIT DEM is also used as the land–sea mask. Monthly temperature (Tmean and Trange are inferred from minimum and maximum temperature) and vapor pressure data from WorldClim V2.1 (Fick and Hijmans 2017) are used to downscale ERA5 from the 0.25° to the target 0.1° resolution because the 1-km WorldClim data contain the topographic information at a very high resolution. WorldClim vapor pressure estimates are converted to Tdew estimates using the Tetens equation (Tetens 1930; Fick and Hijmans 2017). The bias-corrected WorldClim V2 data from the Precipitation Bias Correction (PBCOR) dataset (Beck et al. 2020) are used to correct the undercatch error of EM-Earth precipitation estimates. PBCOR infers the “true” long-term precipitation amount from global streamflow observations using the Budyko curve. The PBCOR WorldClim estimates are spatially aggregated from the raw 0.05° resolution to 0.1° resolution.

Evaluation and comparison datasets.

Some GHCN-D and GSOD stations are not used in SC-Earth and EM-Earth for reasons such as short observation periods, insufficient samples, and failure in gap filling. Those stations have passed quality control and are used as independent data sources to validate EM-Earth ensemble estimates. The station numbers are 33,548, 10,721, and 5,425 for precipitation, Tmean/Trange, and Tdew, respectively. EM-Earth data are also compared to three widely used climate datasets, including the Global Precipitation Climatology Centre (GPCC) dataset (Schneider et al. 2013), the Climatic Research Unit gridded Time Series (CRU TS; Harris et al. 2020), and the University of Delaware Air Temperature and Precipitation Dataset (UDEL; Matsuura and Willmott 2017).

Methodology

Theory of probabilistic estimation.

A meteorological variable at any location and time can be described by a parametric probability distribution (Papalexiou 2018). In this study, the normal distribution [Eq. (1)] is used for temperature variables (Tmean, Trange, and Tdew) and transformed nonzero precipitation (Newman et al. 2015, 2019):
X  N(μ,σ2),
where μ and σ are the mean value and standard deviation, respectively. The methods used to transform precipitation into normal space (Box–Cox and alternative approaches) are summarized in appendix A. Probabilistic estimates can be obtained by randomly sampling from these parametric probability distributions. For precipitation, one more parameter (i.e., the probability of precipitation) is needed to determine if an event occurs. These parameters can be obtained from meteorological estimates and estimation uncertainties, which are produced by optimally merging station and reanalysis data. The detailed steps are introduced as follows.

Deterministic estimation.

Station-based estimates.

Locally weighted linear regression is used as a spatial interpolation method: the topographic attributes at station locations are used as predictor variables in the regression equation, and the meteorological variables at station locations on a given day is the predictand (Clark and Slater 2006). Elevation is a common predictor variable, yet we found that elevation can lead to large bias in regions where the station network is too sparse to represent local topographic variation (e.g., mean temperature is largely overestimated in the Andes Mountains and in the Arctic Archipelago). Therefore, we utilized the climatologically aided interpolation (CAI; Willmott and Robeson 1995) which uses WorldClim climatology as the background and uses locally weighted linear regression to interpolate anomalies (ratio for precipitation and difference for temperature variables). The predictors used in the locally weighted linear regression are latitude and longitude. WorldClim is spatially averaged to the 0.1° spatial resolution and contributes to the inclusion of topographic information in CAI estimates.

The leave-one-out strategy is used to obtain estimates for every station to enable independent evaluation and provide estimates of uncertainty that are used in the optimal interpolation merging strategy (described later). We use the leave-one-out method since it retains the density of stations better than other data withholding methods (e.g., drop 10%) and does not need station selection.

Reanalysis estimates.

The ERA5 estimates are adjusted in time (time shift) to better match the local station data, and adjusted in space (downscaling) to provide estimates at the 0.1° grid.

The time shift of ERA5 optimizes the merging of ERA5 and station data. ERA5 estimates are in UTC, while daily station measurements are often recorded at local time (Yatagai et al. 2020). For example, daily precipitation measurements at manual stations are accumulations referring to the 24 h before the reporting time (e.g., the 24 h before 0700 local time). To account for the temporal mismatch, the hourly ERA5 series is adjusted (i.e., shifted forward or backward) to achieve the optimal agreement between daily reanalysis and station series (appendix B). The temporal adjustment can improve the reanalysis–station-merged estimates, particularly for precipitation that is most affected by the temporal mismatch.

Downscaling the ERA5 data are necessary to provide information at finer spatial resolutions than the original ERA5 grid, which is given at the 0.25° resolution. We downscale ERA5 estimates to obtain 1) 0.1° gridded estimates and 2) point-scale estimates corresponding to stations. The bilinear interpolation is used for precipitation because daily precipitation shows strong spatial variability and advanced statistical downscaling methods are necessary to obtain authentic spatial details. The high-resolution WorldClim is used as the background to downscale Tmean, Trange, and Tdew (appendix C).

Station–reanalysis merging.

Optimal interpolation (OI) is an effective method for multisource merging and can improve the accuracy of gridded estimates (Mahfouf et al. 2007; Xie and Xiong 2011; Fortin et al. 2015; Shen et al. 2018). OI-based merging of station data and ERA5 estimates follows the framework of Tang et al. (2021) with a novel design to calculate spatiotemporally distributed merging weights based directly on observation and background errors (appendix D). OI merging provides gridded meteorological estimates and uncertainty estimates. The leave-one-out strategy is used to validate OI-merged estimates.

We also merge station and reanalysis information to estimate the probability of precipitation using locally weighted logistic regression, which is implemented similar to the locally weighted linear regression. The predictand is the binary precipitation occurrence (0 or 1) from station data, and the predictor is the daily precipitation amount from ERA5 data. The reanalysis–station-merged estimates provide the deterministic version of the EM-Earth.

Probabilistic estimation.

The parameters of the probability distributions in Eq. (1) are generated during the deterministic estimation step. To sample from the probability distributions, we generate the spatiotemporally correlated random field (SCRF; appendix E). The SCRF contains random numbers for every grid and time step. The spatial correlation structure is based on a two-parameter power-exponential correlation function (e.g., Papalexiou and Serinaldi 2020). The temporal correlation structure is based on the lag-1 autocorrelation or intervariable correlation.

Probabilistic estimates are obtained by using the SCRF to sample from the probability distributions (appendix F). We generate 25 ensemble members, which compose the probabilistic version of EM-Earth. A much larger number of ensemble members can be generated, yet to restrict the total size of the EM-Earth dataset we created 25 members.

Postprocessing of EM-Earth.

The postprocessing addresses two problems caused by the limitation of raw station observations: 1) the undercatch of precipitation; and 2) the local reporting time. Station measurements underestimate precipitation amounts due to undercatch of precipitation, particularly for snowfall during windy conditions (Rasmussen et al. 2012). Overcatch may also exist but is ignored here because overcatch is uncommon. We correct EM-Earth deterministic and probabilistic precipitation estimates using PBCOR WorldClim as the background (appendix G). The correction ensures that EM-Earth and PBCOR WorldClim have the same precipitation climatology during their overlapped period from 1970 to 2000, and thus accounts for the undercatch bias and other possible biases.

The raw daily EM-Earth estimates match the local reporting time of meteorological stations, while large-domain applications require data corresponding to 0000–2400 UTC. We use a temporal disaggregation and aggregation method to adjust the reporting time of daily estimates (appendix H). Hourly EM-Earth estimates are obtained during the disaggregation step for all variables except Trange for which hourly data are scarcely used in research and applications. The released version of EM-Earth contains hourly and daily deterministic estimates before and after temporal adjustment, and daily probabilistic estimates after temporal adjustment.

Evaluation of EM-Earth.

Two common metrics, i.e., the correlation coefficient (CC) and the root-mean-square error (RMSE), are used to evaluate EM-Earth deterministic estimates (i.e., OI merging) based on the leave-one-out strategy. We use precipitation estimates before bias correction to match the raw station data. The evaluation uses raw station observations from SC-Earth, although both raw observations and gap-filled estimates are used in the production of EM-Earth. The evaluation of probabilistic estimates uses independent GHCN-D and GSOD stations. The Brier skill score (BSS; Brier 1950) and the continuous ranked probability skill score (CRPSS; Hersbach 2000) are applied to evaluate probabilistic precipitation and temperature estimates, respectively (appendix I). The perfect value for both metrics is one. EM-Earth deterministic estimates are also compared to several widely used deterministic datasets, including GPCC, CRU TS, UDEL, and ERA5 to validate the spatial distributions and climate trends of EM-Earth.

Results

Evaluation of EM-Earth deterministic estimates.

The CC and RMSE of EM-Earth deterministic estimates are shown in Figs. 2 and 3, respectively. The global mean CC values for precipitation, Tmean, Trange, and Tdew are 0.77, 0.97, 0.83, and 0.97, respectively. Natural variability and station density are factors affecting the quality of EM-Earth estimates, particularly for precipitation and Trange that vary more than Tmean and Tdew. All variables show lower CC in the tropics and oceanic islands because of the strong climate variability and lower station density. The CC of precipitation and Trange is lower in Africa, South America, and central and north Asia compared to other regions due to insufficient ground observations.

Fig. 2.
Fig. 2.

The (left) spatial distributions and (right) cumulative density function (CDF) curves of CC for EM-Earth deterministic estimates. CC is calculated using the leave-one-out strategy.

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

Fig. 3.
Fig. 3.

As in Fig. 2, but for RMSE.

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

The global mean RMSE values are 4.50 mm day−1, 1.49°C, 2.50°C, and 1.48°C for precipitation, Tmean, Trange, and Tdew, respectively. The RMSE of precipitation shows higher values in regions where precipitation is larger such as the Amazon rain forest and Malay Archipelago (Fig. 3). Tmean, Trange, and Tdew show lower RMSE in Europe and higher RMSE in central and northeast Asia and the Rocky Mountains in North America. In addition, Tdew shows relatively high RMSE in the Sahara Desert and Arabian Peninsula with a very dry climate. The global mean errors are −0.07 mm day−1, −0.01°C, −0.1°C, and 0.01°C for precipitation, Tmean, Trange, and Tdew, respectively. Overestimation and underestimation coexist in most regions of the world, while a few regions show systematic errors (e.g., Tmean is underestimated in the Sahara Desert and Arabian Peninsula; Fig. ES1 in the online supplemental material). The global mean relative biases of precipitation and Trange are both ∼1% with similar spatial patterns for mean errors (Fig. ES2).

Evaluation of EM-Earth probabilistic estimates.

The spread of probabilistic estimates depends on the uncertainty of deterministic estimates, which show generally consistent spatial distributions with RMSE (Fig. 4). The large uncertainty can result in large spread of probabilistic estimates in regions such as the tropics, South America and Africa for precipitation, and central and northeast Asia for Tmean. The magnitude of uncertainties is related to the precipitation and temperature range. For example, compared to the eastern United States, the western United States shows lower uncertainty in the precipitation magnitude due to the drier climate (Fig. 4), yet it shows a higher ratio of uncertainties due to precipitation estimation issues in the mountains (Fig. ES3). It is challenging for deterministic meteorological datasets to obtain accurate estimates in those regions, while probabilistic estimates can capture the true values through ensemble realizations.

Fig. 4.
Fig. 4.

The spatial distributions of mean daily uncertainty of EM-Earth deterministic estimates from 1950 to 2019.

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

The reliability diagram shows the conditional probability of observed precipitation events given the probability of probabilistic estimates (Fig. 5). The reliability for the 0 mm day−1 threshold is high for all continents. The observed probability is slightly overestimated for the high estimated probability because gridded estimates tend to have more wet events than point-scale station observations. The reliability performance decreases as the rain–no-rain threshold increases from 0 to 50 mm day−1. The rank of the six continents from high to low is North America, Oceania, Europe, Asia, South America, and Africa.

Fig. 5.
Fig. 5.

The reliability diagram of EM-Earth probabilistic precipitation estimates based on independent validation. The estimated probability is derived from 25 EM-Earth ensemble members, and the observed probability is derived from station observations. The threshold for rain–no-rain is shown in the upper-left corner of each panel.

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

The reliability of heavy precipitation estimates is notably worse for Asia, South America, and Africa. In these regions, extreme precipitation events are typically caused by small convective systems. These convective systems are not well captured by the sparse station networks or well simulated by numerical weather models. EM-Earth deterministic estimates have higher accuracy than station-based regression estimates and ERA5 estimates, but could still show a high false alarm ratio and low hit rate for extreme events in Africa, Asia, and South America. The limited number of validation stations is another reason for the poor performance because the reliability performance for large rain–no-rain thresholds may be effected from a few stations located in specific regions. For example, the weak reliability in Asia mainly occurs along the southern slopes of the Himalayas, where the complex topography and climate make accurate precipitation estimation difficult.

Almost all deterministic datasets have low accuracy of heavy precipitation estimates, but probabilistic estimates have advantages in capturing extremes. For example, if EM-Earth deterministic estimates substantially underestimate an extreme precipitation event, most EM-Earth ensemble members will inherit the systematic underestimation resulting in the low reliability (e.g., Fig. 5), however, several members may receive large positive perturbation and thus encompass the true value.

Validation based on BSS and CRPSS metrics (Fig. 6) also shows that EM-Earth precipitation and temperature probabilistic estimates are much better in North America, Oceania, and Europe than in Asia, South America, and Africa. The CRPSS values for Tmean, Trange, and Tdew estimates are particularly high and stable over North America and Europe. For Oceania, the lower rank of temperature estimates compared to precipitation estimates (Figs. 5 and 6) is caused by the larger number of precipitation stations than temperature stations in Australia. South America shows large variation for the 25%–50% CRPSS values (Figs. 6b,d) mainly due to the degraded performance of EM-Earth estimates in the Amazon rain forest.

Fig. 6.
Fig. 6.

Boxplots of (a) BSS for EM-Earth probabilistic precipitation estimates using a threshold of 0 mm day−1, and (b)–(d) CRPSS for EM-Earth probabilistic Tmean, Trange, and Tdew estimates, respectively. The notches, which can roughly denote the significance of difference of medians, equal Q2±1.57(Q3Q1)/n where n is the sample size, and Q1, Q2, and Q3 represent 25th, 50th, and 75th percentiles, respectively. The lower edge, middle line, and upper edge of the box represent Q1, Q2, and Q3, respectively. Values more than 1.5 × (Q3Q1) away from the upper or lower edges (i.e., vertical dotted error range) are outliers (not shown to be clean).

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

Comparison between EM-Earth and other datasets.

EM-Earth precipitation and Tmean are compared to several popular meteorological datasets. Trange and Tdew are not included in this comparison since they are not always provided by existing datasets. We present two types of EM-Earth precipitation estimates: EM-Earth raw and EM-Earth final after bias correction (Fig. 7). The latitudinal curves of precipitation are shown in Fig. ES4. The correction results in a substantial increase in precipitation amounts in high-latitude regions, particularly Greenland. The Malay Archipelago, India, and northern part of South America also see a notable increase of precipitation after correction, indicating that the raw EM-Earth estimates in those regions may be deficient. For example, SC-Earth does not have any stations in the northern corner of South America, resulting in the relatively low quality of EM-Earth and thus obvious correction impact. Compared to GPCC, CRU TS, and UDEL, EM-Earth final shows higher precipitation over most of Asia (particularly the Himalayas), high-latitude North America (particularly Greenland), and Andes Mountains in South America, but slightly lower precipitation in Africa, eastern South America, and Oceania. The phenomenon is consistent with the findings based on PBCOR WorldClim in Beck et al. (2020). ERA5 shows the highest precipitation among all datasets in most parts of the world, particularly South America, East Africa, and mainland Southeast Asia, while in Greenland, ERA5 shows much lower precipitation than EM-Earth final. Nevertheless, EM-Earth final precipitation estimates may not be reliable in Greenland where the PBCOR dataset does not use any streamflow measurement (Beck et al. 2020).

Fig. 7.
Fig. 7.

(a) Mean annual precipitation of EM-Earth final estimates after bias correction, and the differences between EM-Earth final and (b) EM-Earth raw precipitation estimates before correction, (c) GPCC, (d) CRU TS, (e) UDEL, and (f) ERA5. The period is 1950–2019 for all datasets except the UDEL, which is from 1950 to 2017.

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

For Tmean, EM-Earth, CRU TS, and UDEL show the largest difference in Greenland where all datasets lack sufficient observations (Fig. 8). In the Himalayas, EM-Earth Tmean is lower than CRU TS and UDEL but higher than ERA5. In the East Siberian Mountains, EM-Earth is notably higher than CRU TS, slightly higher than UDEL, and slightly lower than ERA5. In the Andes Mountains, EM-Earth is slightly lower than CRU TS, notably lower than UDEL, and slightly higher than ERA5. Overall, all datasets are comparable for Tmean except in some regions with complex topography or very few stations.

Fig. 8.
Fig. 8.

(a) Mean daily air temperature of EM-Earth, and the differences between EM-Earth and (b) CRU TS, (c) UDEL, and (d) ERA5. The period is 1950–2019 for all datasets except the UDEL, which is from 1950 to 2017.

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

GPCC and CRU TS have very similar time series of global annual precipitation and precipitation anomalies from 1950 to 2019 (Fig. 9). ERA5 shows the highest global precipitation and the largest interannual variability. EM-Earth raw precipitation is closer to GPCC, CRU TS, and UDEL after 1970 compared to earlier years (Fig. 9c) because the effect of ERA5 on EM-Earth seems larger in early years when SC-Earth has a high fraction of gap-filled estimates. As the result, EM-Earth shows a larger increasing trend of precipitation compared to other datasets. The mean annual precipitation estimates for global land (excluding Antarctica) are 794, 793, 783, 803, and 862 mm yr−1 for GPCC, CRU TS, UDEL, EM-Earth raw, and EM-Earth final, respectively. EM-Earth final shows the highest precipitation because the PBCOR WorldClim, as the reference for correction, has a global precipitation estimate of 862 mm yr−1, which is close to the Global Precipitation Climatology Project (GPCP) estimate of 853 mm yr−1 (Beck et al. 2020). GPCP uses a different undercatch correction method compared to GPCC and might be closer to the true precipitation in high-latitude regions (Behrangi et al. 2018). For Tmean, all products show consistent interannual variability and trend, except that ERA5 shows a slightly lower Tmean particularly before 1979 probably because the retrospective ERA5 estimates from 1950 to 1978 are still at a preliminary stage.

Fig. 9.
Fig. 9.

Mean annual (a) precipitation and (b) Tmean, along with in (c),(d) their anomalies, respectively. For precipitation, EM-Earth raw and final represent estimates before and after bias correction. GPCC and EM-Earth final do not have data for Tmean.

Citation: Bulletin of the American Meteorological Society 103, 4; 10.1175/BAMS-D-21-0106.1

Many datasets use GPCC or CRU TS estimates as the reference for monthly correction to achieve higher accuracy and consistent spatiotemporal variations (e.g., Huffman et al. 2007; Abatzoglou et al. 2018; Beck et al. 2019). We do not apply such correction to keep the independence of EM-Earth which already integrates information from stations and reanalysis models. Nevertheless, EM-Earth is also suitable for water and energy budget studies that mainly rely on long-term mean climatology data. EM-Earth precipitation data show the same climatology with PBCOR WorldClim due to the bias correction procedure (appendix G). EM-Earth temperature data are close to CRU TS and UDEL in the globe (Fig. 9) and all continents except South America where all datasets show notable discrepancies.

Conclusions

We developed the EM-Earth version 1 dataset with both deterministic and probabilistic estimates of precipitation, Tmean, Trange, and Tdew at the 0.1° resolution for global land areas from 1950 to 2019. Daily minimum and maximum temperature can be estimated from Tmean and Trange since Trange is symmetric about Tmean. Humidity variables such as vapor pressure can be inferred from Tdew estimates. The deterministic estimates are at the hourly and daily scales. The probabilistic estimates are at the daily scale and have 25 ensemble members.

The EM-Earth methodology features several advantages compared to existing meteorological datasets: 1) a serially complete station dataset (i.e., SC-Earth) was developed and used to reduce the effect of stations’ temporal discontinuities on gridded estimates; 2) the temporal mismatch between reanalysis estimates and station observations is considered, which improves the accuracy of EM-Earth estimates (particularly for precipitation); 3) a novel implementation of optimal interpolation is used to merge reanalysis and station data and achieves higher accuracy than using a single input; 4) distributed parameters of spatial and temporal correlation structures are estimated to generate global spatiotemporally correlated random fields; 5) EM-Earth provides both deterministic and probabilistic estimates, and the probabilistic estimates explicitly consider meteorological uncertainties which can complement the inadequacy of existing datasets.

The validation shows that EM-Earth version 1 has reasonable accuracy and comparable distributions and trends with several widely used datasets over the globe. The quality of deterministic estimates is less reliable in regions with complex climate/topography and sparse stations, where probabilistic estimates can provide valuable information of meteorological uncertainties. The dataset can be used in diverse hydrological, meteorological, and climate studies.

Future work will focus on improving precipitation estimates in sparsely gauged regions, including more meteorological variables, and utilizing more data sources. For example, currently, gridded uncertainty estimates are directly interpolated from stations, and EDA ensemble reanalysis estimates could benefit uncertainty estimation in regions with sparse stations. Merging other reanalysis products and satellite products can further improve the quality compared to merely merging ERA5 and station data.

Data availability statement.

The EM-Earth version 1 dataset is available at the Federated Research Data Repository (FRDR) website (https://doi.org/10.20383/102.0547). A link to the entire EM-Earth dataset will be provided upon acceptance of the manuscript.

Acknowledgments.

The study is funded by the Global Water Futures project. SMP acknowledges the support of the Natural Sciences and Engineering Research Council of Canada (NSERC Discovery Grant: RGPIN-2019-06894).

Appendix A: Precipitation transformation

Precipitation at daily or subdaily scales is highly skewed. An appropriate transformation of non-zero precipitation can achieve an approximately normal distribution to enable probabilistic estimation. Here we use the one-parameter Box–Cox transformation with λ = 1/3 (Fortin et al. 2015; Newman et al. 2019; Tang et al. 2021):
{y= xλ1λ x=(yλ+1)λ1,
where x and y are raw and transformed precipitation, respectively. We first generate EM-Earth deterministic estimates using raw precipitation data, and then use the Box–Cox transformation to prepare inputs for the probabilistic estimation. We found that this design achieved better precipitation estimation than directly using transformed precipitation in deterministic estimation because the back transformation introduced biases.

We evaluated alternative probabilistic precipitation estimation methods using the lognormal distribution to replace the normal distribution. The lognormal distribution can directly obtain probabilistic precipitation estimates due to its explicit mathematical expression of the mean and standard deviation. However, probabilistic estimates based on the lognormal distribution were worse than those based on the normal distribution enabled by the Box–Cox transformation (not shown). Future studies can investigate the applicability of parametric probability distributions such as the generalized gamma distribution (Papalexiou 2018; Papalexiou and Serinaldi 2020).

Appendix B: Temporal adjustment of ERA5

The temporal adjustment of ERA5 estimates aims to achieve the highest correlation with station data (Beck et al. 2019). There are four steps. First, hourly ERA5 estimates are matched with stations using the nearest neighbor method. Second, for each station, the matched hourly ERA5 series is shifted by −48, −47, …, 0, …, 47, 48 h, and the daily estimates are obtained for each shift hour. The correlation coefficient between station observations and shifted ERA5 estimates is calculated. The shift hour with the highest correlation is adopted. Third, gridded shift hours are generated by adopting the mode of shift hours of all stations within every country. This is because stations within the same country often adopt the same reporting time, although sometimes different station networks in the same country may have different routines. We do not implement direct interpolation of station-based shift hours because this may introduce large regional uncertainties. Finally, gridded hourly ERA5 estimates are converted to daily estimates based on the gridded shift hours. There is an additional postprocessing step (described in appendix H) to convert the final dataset back to the ERA5 time.

We do not adjust the daily station data using the shift hours because 1) the shift hours may not represent the actual reporting time of stations due to the bias in reanalysis estimates and 2) adjusting raw station data could introduce uncertainties such as inflated wet days and decreased extreme records. The possible historical change of station reporting time (such as in Canada; Hopkinson et al. 2011) is not considered in the study.

Appendix C: Spatial downscaling of ERA5

The downscaling of Tmean, Trange, and Tdew estimates is based on the delta method using WorldClim as the background. First, WorldClim data are averaged from the 1 km to 0.25° resolution. The difference between ERA5 and WorldClim data are calculated at the 0.25° resolution and bilinearly interpolated to the 1-km resolution. Then, WorldClim data are adjusted at the 1-km resolution and averaged to the 0.1° resolution.

The daily 0.1° ERA5 estimates are further downscaled to match meteorological stations. For precipitation, Trange, and Tdew, the nearest neighbor interpolation is used. For Tmean, an additional downscaling step is used because mean temperature generally has a reliable relationship with elevation. We first estimate the long-term monthly temperature lapse rate at the 0.25° resolution based on the regression relationship between vertical ERA5 air temperature and geopotential heights (Tang et al. 2018, 2021). The lapse rate is bilinearly interpolated to the 0.1° resolution and downscale gridded ERA5 estimates to the elevation of matched stations.

Appendix D: Optimal interpolation-based merging

OI-merged estimates are obtained using Eq. (D1):
xA,i=xB,i+j=1mwj(xO,jxB,j),
where xA,i and xB,i are the OI analysis estimate and background estimate for the target grid i, respectively, xo,j and xB,j are the observation field value and background field value for the neighboring station j (j = 1, 2, …, m), respectively, and wj is the OI weight calculated using Eq. (D2):
w(R+B)=b,
where w is the vector of wj(j = 1, 2, …, m), RR and BB are m × m covariance matrices of observation errors and background errors from neighboring stations, respectively, and b is the vector of background error covariance between neighboring stations and the target grid. To solve Eq. (D2), we adopt a novel design proposed by Tang et al. (2021) which explicitly calculates the observation and background errors using two steps: 1) station-based interpolation estimates from the leave-one-out strategy are treated as the observation value (xo), and the difference between interpolation estimates and raw station data are treated as the observation error, and 2) gridded ERA5 estimates are treated as the background value (xB), and the difference between matched ERA5 estimates and raw station data are treated as the background error, which is interpolated to the 0.1°-resolution grids. Given that information, w in Eq. (D2) and xA,i in Eq. (D1) are obtained. This design achieves a tight link between data inputs and OI weights without assuming any empirical error models. The advantage is that OI weights are decided by interpolation and reanalysis quality instead of empirical models fitted in densely gauged regions which are only a small part of the world.

We calculate two types of OI estimates: gridded estimates and leave-one-out strategy-based estimates corresponding to station locations. The second type is used to 1) obtain the gridded uncertainty estimates by interpolating the squared difference between the leave-one-out OI estimates and raw station observations using the inverse distance weighting method, and 2) to perform independent validation of OI-merged estimates.

Appendix E: Generating spatiotemporally correlated random fields

The SCRF is used to perturb deterministic estimates to obtain probabilistic estimates (Clark and Slater 2006). The spatial correlation structure of the SCRF is built on the correlation length function. We compared two exponential functions (Clark and Slater 2006; Svoboda et al. 2015):
{r1p(d)=exp(dc0) r2p(d)=exp[(dc0)s0] ,
where r1p and r2p are correlation functions with one and two parameters, respectively; d is the distance between two points in space; and c0 and s0 are parameters. To obtain globally distributed parameters, each continent is divided into 10° × 10° latitude–longitude boxes. If a box contains fewer than 200 stations, the nearest stations to the box are involved until the minimum number of 200 is met. The three correlation functions are fit for every box and every month. Then, the parameters and coefficients of determination are interpolated to the 0.1°-resolution grids using the nearest neighbor method. For grids with a coefficient of determination smaller than 0.9, the parameters are replaced by parameters from nearest eligible grids. We found that r1p often has relatively low coefficient of determination particularly in tropics, and r2p generally shows coefficient of determination up to 0.95 for all variables and months. Thus, we use r2p in this study.

The temporal correlation between SCRFs at two successive time steps is based on the lag-1 autocorrelation for temperature (i.e., Tmean, Trange, and Tdew) and the cross-correlation between precipitation and Trange (Newman et al. 2015, 2019). The correlation coefficient values are calculated and interpolated in the same way with the parameters of spatial correlation functions.

The SCRF for the first time step is only spatially correlated. For a target grid point, its random number is conditioned on previously generated points using a nested simulation strategy to improve the calculation efficiency (Clark and Slater 2006). The parameters of r2p on the target and previous grids are averaged to generate a new set of parameters. This approach can represent the spatial variability of the spatial correlation structure better than using constant parameters for the whole study area. The SCRF for the following time steps is generated in two steps: 1) a new spatially correlated random field is generated and 2) the field is linked to previous SCRF using Eq. (E2) (Newman et al. 2015):
{Rt,T=ρlag1Rt1,T+1ρlag12Rt1,TRt,P=ρcrossRt,TR+1ρcross2Rt1,P,
where RT and RP are SCRFs of temperature (i.e., Tmean, Trange, and Tdew) and precipitation, respectively; t and t − 1 are the current and previous time steps, respectively; ρlag−1 is the lag-1 autocorrelation of temperature; ρcross is the cross-correlation between precipitation and Trange; and Rt,TR is the SCRF of Trange.

Appendix F: Generating probabilistic estimates

Probabilistic estimates are computed based on the probability distribution in Eq. (1) and SCRF from appendix E (Clark and Slater 2006; Newman et al. 2015). Let R be the SCRF for a specific location and time step, the probabilistic estimate (xT) for temperature (i.e., Tmean, Trange, and Tdew) is
xT=μT+RσT.
For precipitation y in the transformed space (appendix A), we first judge whether an event occurs based on the probability of precipitation 1 − p0, where p0 is the probability of zero precipitation. Let FN(y) be the CDF of the standard normal distribution, FN(R) is the cumulative probability corresponding to the random number R. If FN(R) is larger than p0, the precipitation event occurs and the scaled cumulative probability of precipitation (pcs) is calculated as
pcs=FN(R)p01p0..
The probabilistic estimate of precipitation in the transformed space is expressed as
y={0 if FN(R)p0μP+FN1(pcs)σP if FN(R)>p0.

The estimate y is back transformed to the raw precipitation space using Eq. (A1) to obtain the final probabilistic precipitation estimate (xP).

Appendix G: Undercatch correction of precipitation estimates

Many empirical correction functions are developed to correct the undercatch bias for different types of rain gauges with or without various windshields (Yang et al. 2005; Kochendorfer et al. 2018; Zhang et al. 2019). However, the correction of global precipitation stations is challenging due to the lack of station metadata for SC-Earth and the lack of wind speed observations in many regions. Therefore, we use a simple climatology-based correction method. First, we calculate the long-term monthly mean precipitation from 1970 to 2000 based on EM-Earth deterministic estimates and ensemble mean of 25 probabilistic members. Then, the ratio between EM-Earth and PBCOR WorldClim precipitation is calculated for the period 1970–2000, which is used to scale EM-Earth deterministic and probabilistic estimates from 1950 to 2019.

PBCOR infers precipitation amounts using the water balance method based on the Budyko curve and is affected by the uncertainties in streamflow data (Hamilton and Moore 2012; Kiang et al. 2018), the Budyko curve (Gerrits et al. 2009), parameterization (Beck et al. 2020), noncontributing areas of river basins, and the scarcity of streamflow data in some regions (especially Greenland). Therefore, the current correction scheme is not perfect in this study. In addition, there are other global undercatch correction factors (Adam and Lettenmaier 2003; Yang et al. 2005; Adam et al. 2006) that are not tested in this study. Further efforts are needed to achieve better global undercatch correction by comparing all available methods (water balance–based methods and station-based methods) and datasets.

Appendix H: Temporal adjustment of EM-Earth estimates

The temporal disaggregation and aggregation to obtain EM-Earth estimates at UTC have three steps. First, EM-Earth daily estimates are disaggregated to the hourly scale using the diurnal information of hourly ERA5 estimates after temporal shift (appendix B). The disaggregation uses the multiplicative method for precipitation and the additive method for temperature. Second, the disaggregated hourly estimates are shifted back to the raw ERA5 time routine using the opposite of gridded shift hours obtained in appendix B. Finally, the hourly estimates are aggregated (accumulation for precipitation and average for temperature) to the daily scale corresponding to 0000–2400 UTC. The three steps are implemented for deterministic estimates and each member of probabilistic estimates.

Appendix I: Probabilistic evaluation metrics

The BSS metric is calculated as below:
BSS=1BSBSclim,
BS=1ni=1n(PoPensPoPobs)2,
where BS is the Brier score, BSclim is the climatological BS, PoPens is the estimated probability of ensemble precipitation, PoPobs is the observed precipitation occurrence (0 or 1), and n is the sample number.
The CRPSS metric is calculated as below:
RPSS=1CRPSCRPSclim,
CRPS=[F(x)H(xxo)]2dx,
where CRPS is the continuous ranked probability skill score (CRPS; Hersbach 2000), CRPSclim is the climatological CPRS, F(x) is the CDF of the ensemble estimate x, xo is the observation, H(xxo) is the Heaviside step function (1 for xxo; 0 for x < xo). For a perfect match, the value of CRPSS would be 1. The perfect values are 1 for BSS and CRPSS.

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