1. Introduction
Soil moisture, soil temperature, and vegetation are important land surface variables in the global weather and climate system. Root-zone soil moisture in particular determines the water availability to plants and the partitioning of water into infiltration, runoff, and evapotranspiration. Estimating root-zone soil moisture at the global scale, however, remains a major challenge.
Global estimates of surface soil moisture can be inferred from satellite-based low-frequency passive microwave observations collected by, for example, the current Advanced Microwave Scanning Radiometer 2 (AMSR2) instrument (Imaoka et al. 2010), the Soil Moisture Ocean Salinity (SMOS) mission (Kerr et al. 2010), the Aquarius mission (Le Vine et al. 2007), and the Soil Moisture Active Passive (SMAP) mission (Entekhabi et al. 2010b). However, the utility of spaceborne radiometry is constrained by the limited vertical penetration depth, the coarse spatial resolution, the indirect connection to relevant land surface variables, and the intermittent nature of the measurements.
The assimilation of passive microwave measurements, that is, brightness temperatures (Tb), into land surface models has the potential to add value to these satellite data by (i) increasing the effective vertical penetration depth through propagation of surface information to the root zone (Galantowicz et al. 1999; Crow and Wood 2003), (ii) increasing the spatial resolution through dynamic downscaling (Reichle et al. 2001a), (iii) increasing the spatial and temporal coverage by interpolation and extrapolation to unobserved times and locations (Reichle and Koster 2003), and (iv) providing enhanced and consistent estimates of various land surface state and flux estimates (Crow and Wood 2003). The objective of this paper is to study these benefits, with exclusion of the spatial downscaling (topic of future research), through the direct and joint assimilation of multiangle and multipolarization SMOS Tb into a carefully designed global modeling and assimilation system.
Traditionally, Tb measurements are inverted to soil moisture products prior to use in land surface model applications. The assimilation of soil moisture retrievals in large-scale studies has been beneficial to improve surface and root-zone soil moisture (Reichle and Koster 2005; Liu et al. 2011; Pan et al. 2012; Draper et al. 2012; De Lannoy et al. 2016), as well as other land surface variables (Peters-Lidard et al. 2011; Lievens et al. 2015). However, soil moisture retrievals may be inconsistent with model simulations, as they may utilize different land surface parameters and background information including, for example, vegetation, soil texture, and surface temperature. Furthermore, errors in retrievals will be correlated to errors in the auxiliary (e.g., temperature) information, which in turn can be expected to be correlated with the background information used in the data assimilation system. Such resulting error cross covariances are usually ignored in retrieval assimilation.
It is thus natural to consider a direct assimilation of Tb observations into land surface models. Kalman filters have been used to assimilate Tb at various spatial scales, using either synthetic data (Entekhabi et al. 1994; Reichle et al. 2001a; Wilker et al. 2006; Han et al. 2013; Kumar et al. 2014; Carrera et al. 2015) or radiometer data (Galantowicz et al. 1999; Margulis et al. 2002; Crow and Wood 2003; Huang et al. 2008; Loew et al. 2009; Zhang et al. 2012). Variational Tb assimilation has also been a popular technique (Reichle et al. 2001b; Pathmathevan et al. 2003; Balsamo et al. 2006; Jia et al. 2013; Zhao et al. 2013). The crucial component in these Tb assimilation systems is the inclusion of a radiative transfer model (RTM) as the observation operator to connect the soil moisture, soil temperature, and vegetation characteristics from the land surface model with Tb predictions.
The current paper explores the joint assimilation of SMOS Tb observations at multiple incidence angles, polarizations, and locations at the global scale. While small-scale and synthetic studies have been promising, there can be several reasons why the theoretically more attractive direct assimilation of Tb data may not add the expected value for global applications in practice [e.g., Joiner and Dee (2000) for atmospheric applications]. The benefit of Tb assimilation in continually improving modeling systems depends on a careful treatment of errors in the assimilation system, which may be complex in large systems that simultaneously assimilate multiple observations.
The modeling and assimilation system used in this paper is the Goddard Earth Observing System Model, version 5 (GEOS-5), land data assimilation system, which has the Catchment land surface model (CLSM; Koster et al. 2000) in its core. The GEOS-5 land data assimilation system uses the ensemble Kalman filter (EnKF) and has been used to assimilate a variety of remotely sensed observations separately (Reichle et al. 2014). Recent upgrades to the modeling system include developments in both the land surface model and L-band radiative transfer model (Reichle et al. 2011; De Lannoy et al. 2013, 2014a,b). A variant of this system is used for the operational SMAP Level 4 Surface and Root-Zone Soil Moisture (L4_SM) product (Entekhabi et al. 2014), and this paper can be seen as a first assessment of the system for soil moisture estimation through Tb data assimilation.
The main differences between the multiangular Tb SMOS data assimilation presented in this paper and the SMAP Tb data assimilation performed for the SMAP L4_SM product pertain to the nature of the assimilated Tb observations and the difference in spatial resolution of the end products. SMAP data are collected at one incidence angle and with a relatively small instrument error standard deviation (~1.3 K). In contrast, SMOS provides brightness temperature observations at a range of incidence angles, albeit with a higher instrument error standard deviation (~4 K). The SMOS soil moisture retrieval algorithm thus uses multiangular data (Wigneron et al. 2007; Kerr et al. 2012), as does the assimilation algorithm presented here. Moreover, the estimates from the assimilation system in the present paper are at 36-km resolution, whereas the SMAP L4_SM product provides estimates at 9-km resolution.
Section 2 describes the GEOS-5 CLSM and L-band microwave RTM as well as the SMOS observations and ground validation data. Section 3 discusses the data assimilation system, section 4 lists the experiments and validation metrics, and section 5 presents the results.
2. Observations and model
a. SMOS Tb observations
The SMOS mission provides global Tb data at a nominal (3 dB) spatial resolution of 43 km and with global coverage (at either 0600 or 1800 local time, i.e., ascending or descending half-orbits, separately) approximately every 3 days. The Microwave Imaging Radiometer with Aperture Synthesis (MIRAS) on board SMOS is an interferometric sensor and provides multiangular Tb data at each observed location. Here, we assimilate the multiangular, horizontally H and vertically V polarized Tb observations during the period from 1 January 2010 to 1 July 2014, and we analyze the results from 1 July 2010 to 1 July 2014. The data are extracted from the MIR_SCLF1C product, with processor version 504 for the years 2010 and 2011, and version 505 from January 2012 onward.
The various steps involved in the processing of the multiangular SMOS Tb data are described in De Lannoy et al. (2013) and De Lannoy et al. (2015). The SMOS SCLF1C data are transformed by geometric and Faraday rotation from brightness temperature at the top of the ionosphere and in the antenna reference frame to brightness temperature at the top of the atmosphere and on an Earth-fixed grid. Most importantly, the data are screened extensively using both product-based data quality information and model-based quality control rules (e.g., detection of frozen conditions or heavy precipitation). We limit the Tb data to the exclusively alias-free zone, which leads to relatively narrow swaths and consequently a lower revisit frequency (i.e., global coverage approximately every 6 days for either ascending or descending orbit direction). Data contaminated by radio frequency interference (RFI) are removed when Tb > 320 K or guided by product-based flags. Furthermore, the data are spatially mapped onto the 36-km Equal-Area Scalable Earth Grid, version 2 (EASEv2; Brodzik et al. 2014), and binned per 1° incidence angle. For example, an observation at 40° represents the average of all data with incidence angles between 39.5° and 40.5°. We assimilate swaths of both H- and V-polarized Tb data at seven select incidence angles simultaneously: θ = 30°, 35°, 40°, 45°, 50°, 55°, and 60°. This range of angles adequately samples the angular signature in the brightness temperature signal. Observations at lower incidence angles are not assimilated because of quality concerns in the data version used here (Martín-Neira et al. 2012).
Regardless of the incidence angle, a circular footprint with a 0.22° radius is assumed, which approximates the area of a 36-km EASEv2 grid cell. This is a simplified approach to the actual field of view that is determined by a spatially variable antenna pattern: about 50% of the signal (3 dB) originates from a 43 km × 43 km area, whereas the rest of the signal (with a reduced weight) comes from a larger surrounding area. The weighting by the antenna pattern is included in future SMOS assimilation research and is also implemented for the SMAP L4_SM product.
b. GEOS-5 land surface and radiative transfer model
The simulation of Tb involves (i) land surface modeling with the GEOS-5 CLSM (Koster et al. 2000) and (ii) L-band RTM with a tau–omega model (De Lannoy et al. 2013, 2014b). All simulations are performed with a 7.5-min integration time step, and the computational elements (or tiles) of the modeling system correspond to the 36-km EASEv2 grid cells.
The CLSM version used here is based on the Fortuna 2.5 version of the Modern-Era Retrospective Analysis for Research and Applications (MERRA) with improved land surface variables (MERRA-Land; Reichle et al. 2011), except here we use the 5-cm surface soil moisture layer depth, the new soil parameterization, and the minor code changes of De Lannoy et al. (2014a). The surface layer thus extends from the surface to a depth of 5 cm, the root-zone layer from the surface to a fixed depth of 1 m, and the depth of the entire soil profile varies in space between a global minimum of 1.3 m and a maximum of 8.7 m. Surface meteorological forcing data at a ½° × ⅔° spatial and hourly temporal resolution are taken from MERRA (Rienecker et al. 2011) and bilinearly interpolated to the EASEv2 grid. In some experiments (see section 4), the MERRA precipitation is corrected with gauge-based precipitation from the National Oceanic and Atmospheric Administration (NOAA) Climate Prediction Center “Unified” (CPCU) precipitation product (Reichle 2012; Reichle and Liu 2014).
For each computational element, the CLSM uses three prognostic variables—catchment deficit (catdef), root-zone excess (rzexc), and surface excess (srfexc)—to determine the equilibrium soil moisture profile and deviations from the equilibrium profile in the surface and root zone. The diagnostic surface soil moisture content (sfmc; 0–5 cm) and root-zone soil moisture content (rzmc; 0–100 cm) are calculated from these three prognostic variables along with the saturated, unsaturated, and wilting areas within the tile. In the absence of snow, the surface skin temperature is determined by the area-weighted average temperature across the saturated (tc1), unsaturated (tc2), and wilting (tc4) subtile areas. Finally, the ground heat content (ght1) model prognostic variable determines the soil temperature in the uppermost soil layer (tp1). Further details about the model variables can be found in Reichle (2012), with the difference that the surface soil moisture depth is 5 cm in this paper.
The soil moisture, soil temperature, air temperature, and climatological vegetation dynamics in the CLSM are used as inputs to the diagnostic zero-order (tau–omega) microwave RTM to simulate L-band Tb. Because RTM parameters strongly impact the climatology of simulated Tb, some key RTM parameters were calibrated by minimizing the bias in the mean and variance between long-term SMOS Tb observations and Tb simulations across a set of incidence angles, polarizations, and overpass times (De Lannoy et al. 2013, 2014b). Consequently, the calibrated Tb simulations still show some residual bias at individual incidence angles, polarizations, or overpass times, and the bias typically shows a seasonal evolution. Section 3b discusses how these shorter-term biases are addressed inside the assimilation system. Grid cells without sufficient historical SMOS data for RTM calibration are assigned RTM parameter values based on their dominant vegetation class. These nominal parameter values are calculated as global averages across all calibrated pixels per vegetation class, excluding areas where the soil is classified as peat. In this study, the RTM calibration is done over the same 4-yr period as the assimilation experiments. The calibration minimizes climatological biases (De Lannoy et al. 2013), whereas the assimilation addresses random (or short term) errors.
c. Ground validation data
The assimilation results are validated during the period from 1 July 2010 to 1 July 2014, using independent in situ observations of surface and root-zone soil moisture, as well as surface soil temperature from sparse networks in the United States, Australia, and Europe, and from intensively monitored validation watersheds (Entekhabi et al. 2014) in the United States. All data are subjected to intensive quality control to remove irregularities or sensor trends as discussed in Entekhabi et al. (2014) and De Lannoy et al. (2014a).
The sparse networks include the U.S. Natural Resources Conservation Service (NRCS; Schaefer et al. 2007) Soil Climate Analysis Network (SCAN), the U.S. Climate Reference Network (USCRN; Diamond et al. 2013; Bell et al. 2013), the Oznet network in Australia’s Murrumbidgee catchment (Smith et al. 2012), and the SMOS–Meteorological Automatic Network Integrated Application (SMOSMANIA) in France (Albergel et al. 2008; Dorigo et al. 2011). The advantage of SCAN and USCRN is that they offer extensive ground data of soil moisture and temperature in both the surface and root zone and across a variety of climatological conditions and land surface characteristics. The Oznet and SMOSMANIA sites cover a smaller domain, but complement the validation in different continents.
Surface soil moisture measurements are taken at approximately 5 cm depth. For SCAN and USCRN sites, root-zone soil moisture measurements are a weighted average of measurements at 5, 10, 20, and 50 cm depth. For Oznet and SMOSMANIA sites, root-zone measurements are extracted at 45 and 30 cm depth, respectively, for lack of sufficient data in other layers. For SCAN and USCRN, sites missing data in any of the root-zone layers are excluded, even if good surface measurements would be available for surface soil moisture validation. In contrast, for the Oznet and SMOSMANIA networks, no cross masking between the surface and root-zone validation is included because of data limitations. Surface soil temperature is validated separately.
Unless noted otherwise, validation sites are limited to “favorable” areas, that is, to areas where the relationship between Tb observations and soil moisture is relatively straightforward. Sites are excluded from this category where the maximum climatological Moderate Resolution Imaging Spectroradiometer–based leaf area index (Mahanama et al. 2015) exceeds 5, or if they are within 36-km grid cells that are predominantly covered by forest or shrubland according to the International Geosphere–Biosphere Programme vegetation classification. Finally, sites are excluded in areas with complex topography (determined from GEOS-5 parameters based on HYDRO1k data; Verdin and Jenson 1996) or if the site elevation differs by more than 500 m from the mean elevation of the 36-km grid cell.
The point validation is complemented with a validation using gridcell-scale in situ data, referred to as data in “reference grid cells.” In a few U.S. Department of Agriculture (USDA) watersheds across the United States, dense local networks of sensors were installed to calibrate and validate coarse-scale remote sensing observations (Cosh et al. 2008; Jackson et al. 2010). The measurements from these watersheds are part of the core validation sites used to evaluate SMAP data products (Entekhabi et al. 2014). Table 1 lists 10 reference grid cells (36 km) within six USDA watersheds. Each reference grid cell has a minimum of five individual sensors measuring surface soil moisture for at least 2 years during the validation period. Only 5 of the 10 reference grid cells also have root-zone soil moisture measurements. The lengths of the data records vary but cover most of the 4-yr validation period, except for South Fork, where the record is limited to 2 years.
The 36-km reference grid cells within SMAP core validation watersheds (Entekhabi et al. 2014). Each reference grid cell contains a minimum of five surface soil moisture sensors and a maximum of N sensors. The latitude and longitude refer to the center of the EASEv2 36-km grid cells. Sites marked with an asterisk also provide measurements in the root-zone layer.
3. Data assimilation
a. Distributed ensemble Kalman filter
The EnKF system simultaneously assimilates a set of multiangular, H- and V-polarized SMOS Tb observations (each with a footprint radius of 0.22°) located within a circular area with a 1.25° radius around each 36-km model grid cell. The differences between these multiple Tb observations and their modeled counterparts are used to update the relevant underlying land surface model state variables at each 36-km model grid cell. A schematic of the data assimilation system is shown in Fig. 1.
The distributed or three-dimensional (3D) EnKF has been used in earlier land surface data assimilation experiments (Reichle and Koster 2003; De Lannoy et al. 2010; Sahoo et al. 2013). These earlier studies include both spatial smoothing and downscaling of coarse observations to the finer model resolution as part of the 3D filter, whereas in this paper the observation and the model grid resolution are similar (model resolution, EASEv2 36 km; observation footprint radius, 0.22°) and the 3D filter mainly serves for spatial interpolation and extrapolation. The downscaling to a finer (9 km) resolution to support the SMAP L4_SM product (Entekhabi et al. 2014) will be discussed in future research.
The EnKF system is designed to update root-zone soil moisture in response to observations that are mainly related to surface soil moisture. Thus, root-zone soil moisture increments rely on ensemble error correlations between the surface and root zone. Root-zone soil moisture estimates from the analysis are also informed through vertical propagation of surface increments, which depends on the vertical coupling strength in the CLSM (Kumar et al. 2009). The distributed analysis also enables soil moisture and soil temperature updates at unobserved times and locations, so that soil moisture and temperature are updated more frequently than at every overpass. A spatially smooth analysis is ensured through spatially correlated forecast errors, which are suppressed in locations that are farther removed from the analysis grid cell.
b. Biases
The Kalman filter assumes unbiased Tb observations and forecasts, and thus unbiased innovations. Even after RTM calibration, however, there are residual biases between SMOS Tb observations and GEOS-5 Tb forecasts that vary with season, incidence angle, polarization, and orbit direction (or overpass time). It is not yet clear how to adequately partition these biases into observation and forecast bias or how to come up with appropriate bias models to guide dynamic bias updates (De Lannoy et al. 2007; Reichle et al. 2010; Pauwels et al. 2013; Draper et al. 2014) at the global scale. Therefore, we rely on historical records of the SMOS Tb observations and the corresponding ensemble mean GEOS-5 Tb forecasts to remove seasonally varying climatological bias in the Tb innovations prior to data assimilation.
Figures 2a and 2b illustrate differences between climatological ensemble mean Tb simulations and SMOS observations at 40° incidence angle on pentad 36 (from 27 June to 1 July) for ascending Tb at H polarization and descending Tb at V polarization. The bias is very different for each combination of incidence angle, orbit, and polarization because the RTM was calibrated so that the long-term bias across all assimilated Tb observation types would be minimal. In exceptional areas like the Sahara Desert, a known cold model bias is found across all Tb types on average. Figures 2c and 2d further illustrate that the climatological bias at individual locations also varies in time. Figure 2 is produced using ensemble open-loop (model only, no assimilation) simulations without CPCU precipitation corrections (section 2b). The bias is slightly smaller when CPCU corrections are used.
Note that for soil moisture retrieval assimilation, innovation biases are often removed through cumulative distribution function matching (Reichle et al. 2004), where long-term higher-order statistics of observations and simulations are matched, regardless of the time in the year. In addition to its sensitivity to soil moisture, brightness temperature also depends strongly on the land surface temperature and on vegetation characteristics, both of which typically have a strong seasonal cycle. Bias in brightness temperature therefore varies seasonally, and its correction must also depend on the season. We therefore use a seasonally evolving climatological mean adjustment.
c. Forecast errors
The forecast error covariances
Ensemble perturbations to forcing and model prognostic variables. The perturbation type is either additive A or multiplicative M, with the standard deviation given for a normal or lognormal distribution, respectively. The time series correlation (temporal correlation) is applied to a first-order autoregressive model. The spatial correlation scale (spatial correlation) is isotropic. Perturbations to prognostic variables are uncorrelated with each other and with the forcing perturbations.
The prognostic state variables catdef and srfexc (related to soil moisture) are perturbed to mimic errors in model structure and model parameters. Prognostic variables related to surface (skin) and soil temperature are not perturbed explicitly to avoid excessive temperature updates, but a limited uncertainty in temperatures is implicitly created through the perturbation of the radiation and other forcings. Yet, over dry areas with limited vegetation (e.g., Sahara Desert), the perturbation in radiation may still result in a large temperature spread.
The perturbations to the model prognostic variables are additive with a temporal correlation length of 3 h, a spatial correlation length of 0.5°, and no cross correlations. However, weak cross correlations will develop through balancing during the model simulation; explicitly correlated perturbations to catdef and srfexc were found to excessively update root-zone soil moisture. A new sample of perturbations is calculated every 3 h and then interpolated and applied at every model time step (7.5 min). During the state updating, spurious long-range forecast error correlations are suppressed beyond 1.25°, that is, 2.5 times the spatial correlation length, using a Hadamard multiplication of the sample error covariance terms with a distance-dependent and compactly supported function (Reichle and Koster 2003; Gaspari and Cohn 1999). This localization limits the complexity of the Kalman gain inversion and effectively selects only observations located within a 1.25° radius around the analysis grid cell for assimilation.
Spatially and temporally correlated forcing and state perturbations will cause correlated state forecast errors. The filter adequately accounts for the spatial error correlations by performing a smooth spatial state update. In contrast, despite the temporal correlations, updates are only calculated at single instants, because the land surface model and filtering only rely on the last update to compute the next forecast.
Whereas the perturbation parameters are constant in space and time, the resulting spread in soil moisture and temperature show distinct spatial and temporal patterns, corresponding with the magnitudes of the respective variables. The resulting uncertainty in Tb observation predictions
d. Observation errors
The observation error covariance matrix
4. Experiments and validation
a. Experiments
The experiments consist of two ensemble open-loop experiments (model only, with perturbations) and two corresponding data assimilation experiments (with the same perturbations as the open loop) as listed in Table 3. The first set is performed without and the second set with CPCU precipitation corrections (section 2b). The simulations without precipitation correction are used to study the expected impact of data assimilation in areas without dense precipitation gauges, such as in Africa or central Asia. This approach is in line with Liu et al. (2011), where the relative impact of soil moisture assimilation and precipitation corrections was studied. The open-loop experiments are denoted as OL and OLPcp, without and with precipitation corrections, respectively. The data assimilation experiments are denoted as DA and DAPcp, without and with CPCU precipitation corrections, respectively.
Overview of experiments.
b. Validation metrics
The skill of the assimilation results is assessed using 4-yr time series of 3-h averaged surface and root-zone soil moisture and surface soil temperature extracted at 36-km grid cells that either contain the point sites of the sparse networks or correspond to reference grid cells (section 2c). We include all time steps for which in situ observations are available, regardless of whether Tb was assimilated or not at a given time and location. Skill metrics are calculated for the entire period from 1 July 2010 to 1 July 2014 and separately for the central 5 months in the warm season of the same 4-yr period. For the validation sites in the Northern Hemisphere, the warm season includes May–September; for the Oznet sites, the warm season includes November–March. For surface soil temperature, the validation is limited to the warm season only and metrics are calculated separately for each 3-h time interval (0000–0300, 0300–0600, …, 2100–2400 UTC) before computing an average metric across the eight 3-h time intervals. This procedure avoids that diurnal effects would otherwise dominate the skill metrics. Furthermore, it will be shown that surface soil temperature updates have only a limited memory, and differences in temperature skill are thus best detected when the metric is limited to the warm season, that is, when Tb observations are actually assimilated (over nonfrozen land). Frozen or snow-covered conditions are always excluded.
Skill is measured in terms of time series correlation R, anomaly time series correlation (Ranom), unbiased root-mean-square difference (RMSDub; Entekhabi et al. 2010a), and bias. The Ranom is calculated as the time series correlation coefficient between the simulations and ground observations after removal of their respective seasonal climatologies. The climatology is calculated for each 3-h time interval of each day of the year as the 4-yr average of the smoothed time series (smoothing window = 31 days) of data points at that particular 3-h time interval. In contrast, the RMSDub is obtained after removal of the static long-term mean bias between the simulations and the ground observations. The RMSDub can also be interpreted as the temporal standard deviation in the errors between in situ observations and simulations.
Skill metrics are only calculated if at least 200 data pairs are available for validation. The 95% confidence intervals assume a Student’s t distribution for the bias and mean-square difference (MSD),
5. Results
a. In situ validation
1) Sparse networks
Figure 3 shows the Ranom for the two open-loop experiments (OL, OLPcp) and the two assimilation experiments (DA, DAPcp), averaged across the SCAN and USCRN sites in favorable locations (section 2), and for the entire period from 1 July 2010 to 1 July 2014. For the SCAN surface soil moisture, the average Ranom is 0.46 and 0.55 (unitless) for open-loop simulations OL and OLPcp, respectively. With assimilation, the Ranom values increase to 0.63 and 0.66 for experiments DA and DAPcp, respectively. Improvements are also found in the root zone, where the Ranom is 0.53 and 0.63 for OL and OLPcp and the Ranom increases to 0.64 and 0.66 for DA and DAPcp, respectively. For surface soil temperature, the improvements are small by design (section 3c), but statistically significant. At the USCRN sites, the findings are very similar. As expected (Reichle et al. 2011), the use of gauge-based precipitation data (OLPcp, DAPcp) yields soil moisture simulations that are in better agreement with in situ soil moisture observations than simulations that are not informed about in situ precipitation observations (OL, DA).
The improvements in Ranom due to Tb assimilation are comparable to those found in earlier studies where retrievals from AMSR-E, ASCAT, or SMOS (Liu et al. 2011; Draper et al. 2012; De Lannoy et al. 2016) were assimilated in earlier versions of the GEOS-5 CLSM. The SMOS Tb assimilation is able to add information that is complementary to the recent improvements in the modeling system (De Lannoy et al. 2016), even with superior precipitation forcings. Yet, unlike in Liu et al. (2011), here the improvements due to Tb assimilation are smaller when precipitation corrections are used. However, it is difficult to compare the improvements across the various studies, because the metrics and confidence intervals also depend on the experiment period and the temporal resolution of the validation time series.
Figure 4 shows maps for the change in Ranom between the open-loop simulation and Tb assimilation experiment without precipitation corrections [ΔRanom = Ranom(DA) − Ranom(OL)] at individual SCAN and USCRN sites in favorable locations as indicated by the green background shading, for the period from 1 July 2010 to 1 July 2014. The number of validation sites used here is limited because of the need to estimate the climatology robustly. Moreover, the significance of the changes is limited, especially for root-zone soil moisture, because of the relatively strong autocorrelation in the root-zone soil moisture time series. Despite these limitations, the figure shows that surface soil moisture is improved at almost all sites (92 out of 100) with a cluster-averaged ΔRanom = 0.12, while root-zone soil moisture is improved at a majority of sites (70 out of 100) with a cluster-averaged ΔRanom = 0.05. At a few sites, a degradation can be attributed to an erroneous quantification of the vegetation in the RTM or an inadequate horizontal propagation of information.
Table 4 summarizes the skill of soil moisture and temperature estimates for all sparse networks, limited to favorable locations and to only the four warm seasons for each network. Brightness temperature assimilation is expected to have the most impact on soil moisture estimation when the land is not frozen. The metrics are very similar for SCAN, USCRN, Oznet, and SMOSMANIA, with generally higher Ranom values for experiments with CPCU corrections than those without CPCU corrections. The Ranom for the assimilation experiments is always better than the open-loop simulations. The improvements are only statistically significant for SCAN and USCRN in terms of surface soil moisture and, in the absence of CPCU precipitation corrections, also for root-zone soil moisture at SCAN sites (ΔRanom = 0.12). Substantial improvements are found for Oznet and SMOSMANIA, but given the limited time period and the limited spatial coverage of these sites, these improvements are not statistically significant.
Skill metrics at SCAN, USCRN, SMOSMANIA, and Oznet sites, with indication of the half value of the 95% CIs averaged over all experiments (for asymmetric CIs, the mean half value is shown). The metrics are calculated using all 3-hourly time steps during the warm season across 4 years. Variable N is the number of sites for each network, with the number of clusters in parentheses. Clusters are not used for the Oznet and SMOSMANIA sites, where the CIs are conservatively estimated as the simple average of the CIs over individual sites. Temperature validation is not performed at the Oznet sites for lack of sufficient data pairs at each individual 3-h time interval.
Especially in terms of RMSDub, the skill for root-zone soil moisture is always better than that of surface soil moisture (Table 4) because root-zone soil moisture is less variable. Data assimilation reduces the RMSDub in both the surface and root zone for all networks, but as already noted above, the assimilation has fewer opportunities to add complementary information when CPCU precipitation corrections are used. The table further shows that the surface soil temperature skill is not altered through Tb data assimilation, because temperature updates only have a limited memory.
The above validation is constrained to areas with moderate topographic complexity and limited vegetation based on coarse-scale model parameters. A detailed investigation of the Tb data assimilation in more complex areas is beyond the scope of this paper. However, it should be mentioned that soil moisture updates are found under relatively dense vegetation, where Tb observations are rather insensitive to soil moisture. The soil moisture updates under vegetation can be explained by a combination of the spatial propagation of information from less vegetated areas and the relatively high ensemble soil moisture spread in wetter, vegetated areas (because the larger forecast uncertainty in these areas results in larger increments).
Figure 5 shows the changes in RMSDub [ΔRMSDub = RMSDub(DA) − RMSDub(OL)] for the experiments without precipitation corrections, for all sites with sufficient root-zone data in either favorable or unfavorable areas during the entire period from 1 July 2010 to 1 July 2014. The green background again identifies the areas with limited vegetation and topographic complexity, whereas white areas mark complex terrain or (seasonal) dense vegetation.
For the joint SCAN and USCRN, 63% of all sites show an improvement in root-zone soil moisture. A solid improvement is found for most sites in the Great Plains (e.g., Oklahoma, Kansas, Nebraska, and the Dakotas), whereas degradation is found in the western mountainous areas (e.g., Utah, Nevada) where root-zone soil moisture is difficult to measure and simulate. Surface soil moisture is improved at 77% of the SCAN and USCRN sites, with large improvements in the Great Plains and minor improvements still found in the western half of the United States (not shown).
Improvements in the root-zone soil moisture estimates are also found at 72% of the Oznet sites and at 65% of the SMOSMANIA sites (Fig. 5). Model soil moisture at most Oznet sites is updated frequently because SMOS observations are abundant in this area (section 5b). Especially in the Yanco area (largest cluster in Fig. 5b), most sensors show improved root-zone soil moisture. Similarly, the RMSDub in the surface soil moisture is decreased by more than 0.01 m3 m−3 at the Oznet sites (not shown). In contrast, the impact of the assimilation is very small at the SMOSMANIA sites in both surface (not shown) and root-zone soil moisture, regardless of the location. This is mainly due to the limited number of SMOS Tb data used to update soil moisture, because in this area data are often screened out because of frozen conditions, heavy precipitation, or RFI. The spatial filter may also propagate information from the nearby Pyrenees Mountains into the Piedmont region where the sensors are located, which may not always be beneficial for the estimation of local conditions.
2) Reference grid cells
The skill of the OL, OLPcp, DA, and DAPcp experiments at the reference grid cells is shown in Fig. 6 for the Ranom and in Fig. 7 for RMSDub, bias, and R. Figure 6 shows that the assimilation generally increases the Ranom for surface and root-zone soil moisture, as well as for surface soil temperature for all reference grid cells. The exception is South Fork, where the in situ data record only covers 2 years, artificial drainage installed for agriculture complicates the interpretation of the soil moisture validation results, and insufficient data are available for temperature validation. The average improvement (ΔRanom) for surface soil moisture is 0.18 without precipitation corrections and 0.08 with precipitation corrections (statistically significant). Without precipitation corrections, these changes are similar to the ΔRanom = 0.16 reported in Liu et al. (2011) when assimilating a long time series of AMSR-E soil moisture retrievals into an older version of the GEOS-5 CLSM. Yet, in contrast to Liu et al. (2011), the Tb assimilation in the updated system here yields smaller improvements when superior precipitation forcings are used. Presumably, the reason for this result is the fact that here we use an improved modeling system. Moreover, the length of the time series used here is shorter, making it more difficult to discern statistically significant improvements.
Figures 7a and 7d show that the open loop without precipitation corrections (OL) yields an RMSDub of 0.042 m3 m−3 for the surface and 0.039 m3 m−3 for the root-zone soil moisture across all reference grid cells. With assimilation (DA), the RMSDub reduces to 0.036 m3 m−3 for the surface and 0.033 m3 m−3 for the root zone, across the available reference grid cells. When including precipitation corrections, the RMSDub for the open loop (OLPcp) is 0.038 m3 m−3 for the surface and 0.033 m3 m−3 for the root-zone soil moisture across all reference grid cells. With assimilation (DAPcp), the RMSDub reduces to 0.034 m3 m−3 for the surface and increases slightly to 0.034 m3 m−3 for the root zone.
The assimilation slightly decreases the RMSDub in surface soil temperature (not shown) at all reference grid cells except South Fork, which is a combined effect of directly updating the soil temperature and changes in fluxes resulting from soil moisture updates. On average, the RMSDub for the open loop and data assimilation experiments is around 2 K, with higher values (3.5 K) in Walnut Gulch and lower values (1.2 K) in Little River (not shown).
Figures 7b and 7e show the bias values for surface and root-zone soil moisture. The local bias is larger than the RMSDub, which is expected, when considering that the global land surface model relies on ancillary information for texture and vegetation. With CPCU precipitation corrections, the bias is slightly larger than without such corrections. This was also found for SCAN and USCRN sites (not shown). By design, the assimilation changes the bias only minimally (except in South Fork, where the validation period is too short) and these small changes can be attributed to the spatial nature of the filter. The Tb assimilation further introduces a significant improvement in R for the surface soil moisture (Fig. 7c). For the root zone, the improvement in R due to Tb assimilation alone is not statistically significant (Fig. 7f) because of the limited time period, but the improvement is as high as 0.23 when no CPCU precipitation corrections are used.
As an example, Fig. 8 shows soil moisture time series for experiments OLPcp and DAPcp along with in situ observations at Fort Cobb for each July and August in the 4-yr experiment period. Because of Tb assimilation, the responses to the precipitation events of July 2010 and August 2013 are better simulated in the root zone. In August 2010, the SMOS observations are anomalously warm relative to a 4-yr climatology, suggesting drier-than-usual conditions. The assimilation thus changes surface and root-zone soil moisture toward the in situ observations. Some irregularities in the surface soil moisture indicate that some updates may be too strong, because the observation error standard deviation of 6 K may be too low at this location.
b. Large-scale results
In this section, global assimilation diagnostics at the 36-km model resolution are presented to evaluate the quality of the multiangular SMOS Tb assimilation system. Only simulations with CPCU precipitation corrections are presented for simplicity.
1) Innovations (observation space)
Figure 9a shows a map of the average number of (ascending or descending) half-orbits per day for which SMOS Tb observations of at least one polarization and incidence angle were assimilated. On average, there is one set (multiangle, two polarizations) of Tb observations every 3 days (or every 6 days per orbit direction, see also section 2a), with fewer data available in mountainous and northern areas with prolonged freezing conditions. Because of RFI contamination, data are missing in large portions of Asia, eastern Europe, and the Middle East.
The temporal mean in the bias-corrected (section 3b) Tb innovations is close to 0 K by design (not shown). The temporal standard deviations in the normalized Tb innovations
Figure 9b shows that experiment DAPcp leads to areas where the metric is much smaller or larger than 1. For example, in the central agricultural area of the United States, the standard deviation of the normalized innovations is larger than 1, which indicates that the DA system underestimates Tb observation and/or forecast errors. The calibration of the RTM (De Lannoy et al. 2014b) revealed higher errors in Tb predictions over cropland, and consequently, it can be expected that
2) Increments (state space)
Figure 10a shows the average number of increments per day applied at each location during the four validation years. Increments are counted when a value larger than 10−5 mm is found for any soil moisture component (catdef, srfexc, rzexc) or a value larger than 10−3 K for surface soil temperature. In observed areas, increments are applied every 1–2 days, which is more frequently than the number of overpasses per day (Fig. 9a). The 3D EnKF effectively applies increments outside the observed swaths (up to a spatial error correlation localization distance of 1.25°) and in areas where observations are not available or screened out after quality control. It should be noted that the number of increments varies seasonally, with most increments during the summer and a reduced number of increments in the winter.
Figure 10b shows the temporal standard deviation in the increments to the total soil water column (prmc), expressed in volumetric fractions (i.e., accounting for variable profile depths), for the assimilation experiment DAPcp. Similarly, Fig. 10c shows the standard deviation in the surface soil temperature (tp1) increments. Not shown are the mean increments, which are negligible, because the system is nearly unbiased by design. The standard deviation in the increments is small when spatially and temporally averaged, because many very small increments are associated with distant observations (3D EnKF). This is especially true in coastal areas where updates are solely related to distant observations (because Tb observations near water are removed during quality control). For experiment DAPcp, the temporal standard deviation in prmc increments amounts to 3.8 × 10−3 m3 m−3 for the globe (Fig. 10b), with some areas showing distinctly larger or smaller absolute increments. The larger increments are often associated with underestimated observation errors (Fig. 9b). The global average of the surface soil temperature increments is 0.65 K, with higher values in drier areas with limited vegetation and Tb forecast uncertainties that are perhaps too large because of excessive temperature uncertainties. The temporal standard deviation in the temperature and moisture increments is larger in the summer and reduced in the winter (not shown).
3) Other variables
Next, we analyze the impact of Tb data assimilation on other land surface variables, including the latent and sensible heat fluxes and runoff, across the globe (Fig. 11) and for North America (20°–50°N; Table 5). Figure 11 measures impact in terms of the RMSD between the open loop (OLPcp) and the assimilation integration (DAPcp) over the 4-yr time series. For North America only, Table 5 provides the long-term mean and standard deviation values of the OLPcp simulation and differences from the corresponding DAPcp values separately for each season and for the entire year. Table 5 also provides the RMSDub values between OLPcp and DAPcp. Table 5 shows very small differences (bias) in (absolute) long-term means and standard deviations for most variables, which implies that the RMSD is close to the RMSDub.
Spatial average of the long-term and seasonal [December–February (DJF), March–May (MAM), June–August (JJA), and September–November (SON)] statistics for experiment OLPcp and differences with experiment DAPcp for various land surface variables. The OLPcp statistics include the temporal mean (mean OLPcp) and standard deviation (std dev OLPcp). Difference statistics include the difference in the mean, mean of the absolute differences, difference in the standard deviation [MDiff, MabsDiff, and SDiff (DAPcp minus OLPcp), respectively], and the RMSDub between DAPcp and OLPcp results. Statistics are calculated as the spatial average of the metrics for North America (20°–50°N) during the period from 1 Jul 2010 to 1 Jul 2014.
The globally averaged RMSD values between OLPcp and DAPcp are very small (Fig. 11), because some regions do not receive any updates for lack of Tb observations of sufficient quality (section 2a). For surface and root-zone soil moisture, the values of the global RMSD are 0.02 and 0.01 m3 m−3, respectively (Figs. 11a,b). The RMSD is higher in northern latitudes where the CPCU precipitation corrections are tapered (no corrections above 62.5°N) and data assimilation has more impact. When focusing on North America, which is well observed by SMOS, Table 5 reveals that the RMSDub per season amounts to less than 10% of the open-loop mean soil moisture, but to around 50% of the open-loop standard deviation. As expected, the RMSDub in surface soil temperature is very small and only amounts to about 5% of the open-loop standard deviation.
The RMSD between OLPcp and DAPcp in the energy fluxes has values of about 9–10 W m−2 across the globe for sensible and latent heat, with more pronounced effects in the central United States and the Southern Hemisphere. Table 5 indicates that the RMSDub in energy fluxes is about 20% of the mean open-loop values and about 10%–20% of the mean temporal standard deviation, with larger changes in the summer and fall months.
The RMSD between OLPcp and DAPcp in total runoff is about 0.27 mm day−1 across the globe (Fig. 11f) with large RMSD values in the wetter eastern part of North America, where most of the soil moisture updates are applied. The RMSDub values for North America (Table 5) reach up to 80% of the mean seasonal values and reach up to 20% of the temporal standard deviation in the fall months. Figure 11f shows very high RMSD values over the Amazon and the Indonesian archipelago, where the model produces very high runoff peaks. Small updates in soil moisture over these areas result in large absolute changes in runoff, but the changes are small relative to the magnitude of the runoff.
4) Uncertainty
One of the advantages of the EnKF is its ability to provide ensemble error estimates for simulated variables. Figures 12a, 12c, and 12e show the analysis error standard deviation in soil moisture and surface soil temperature for the assimilation integration DAPcp (enstda), averaged over all 3-hourly time steps from 1 July 2010 to 1 July 2014. The estimated uncertainty in surface soil moisture is about 0.02 m3 m−3 across the globe and higher in areas with limited or no assimilation updates (e.g., Asia, northern latitudes). The uncertainty is also high, for example, in the dry western United States and the dry Sahara desert, where surface soil moisture regularly drops below the wilting point, the transpiration stops and the replenishment by the root zone is halted. This makes the surface soil moisture more sensitive to surface meteorological perturbations, whereas the uncertainty in root-zone soil moisture remains limited (Fig. 12c). The latter explains why these dry areas still show small absolute profile soil moisture increments (Fig. 10b). The uncertainty in the root-zone soil moisture is globally smaller (about 0.01 m3 m−3 across the globe; Fig. 12c), because the uncertainties in the forcings are dampened. For soil temperature, the ensemble uncertainty is mostly less than 1 K and limited by design (section 3c), but high temperature uncertainties are found in dry areas with limited vegetation. Some coastal grid cells show a high uncertainty, because the assimilation only affects these locations through small updates based on distant Tb observations.
Figure 12 also verifies the expectation that data assimilation reduces the uncertainty of the estimated land surface variables. Specifically, Figs. 12b, 12d, and 12f show the ratio of the temporal mean ensemble standard deviation for the assimilation integration DAPcp (enstda) to the ensemble standard deviation in the model-only open-loop simulation OLPcp (enstdm). Again, the ensemble standard deviations are averaged across all 3-hourly time steps from 1 July 2010 to 1 July 2014. For surface soil moisture, the averaged ratio is 0.85 across the globe. In some wetter and well-observed areas, the estimated uncertainty is halved by the assimilation (e.g., parts of the central United States), whereas the uncertainty is only marginally changed in boreal regions and unaltered across much of Asia and southeastern Europe where no observations are available for assimilation. In some areas with dense vegetation and where Tb is only marginally sensitive to soil moisture, for example, in central Africa, the uncertainty is only marginally changed. The root-zone soil moisture shows a similar pattern, but with a greater reduction in uncertainty, that is, a ratio of 0.74 across the globe. The reduction is greater than in surface soil moisture, because root-zone soil moisture has a longer memory and is less directly exposed to perturbations in the meteorological forcings. In terms of surface soil temperature, only a minor contraction of the ensemble spread is noticed when averaged across all 3-hourly time steps, because of the limited memory of (surface) soil temperature updates in the modeling system.
6. Conclusions
The direct assimilation of multiangle and multipolarization SMOS Tb observations into the GEOS-5 land surface model is evaluated for global soil moisture estimation. The assimilation uses a distributed ensemble Kalman filter with a temporally variable Tb bias mitigation, a system that is also used for the SMAP L4_SM product. The distributed aspect of the filter introduces updates that are spatially extrapolated into unobserved areas. The multidimensional aspect of the observations is a unique feature of this paper: for each location on Earth, several hundreds of SMOS Tb observations may be assimilated simultaneously.
Two types of assimilation experiments are performed, one using MERRA forcings and one using MERRA forcings corrected with CPCU gauge precipitation. In both cases, the multiangular SMOS Tb assimilation yields better results than an open-loop simulation in terms of the anomaly time series correlation (Ranom) and unbiased root-mean-square difference (RMSDub). Improvements are found in both the surface and root-zone soil moisture for sites in sparse networks (SCAN, USCRN, SMOSMANIA, Oznet) and reference grid cells across the United States, limited to areas with mild topography and limited vegetation. The Tb data assimilation thus effectively helps to propagate surface information to the root zone. The magnitudes of the improvements in Ranom due to SMOS Tb assimilation are comparable to what is reported in studies assimilating longer time series of soil moisture retrievals from AMSR-E or Advanced Scatterometer (ASCAT) in older versions of the GEOS-5 CLSM (Liu et al. 2011; Draper et al. 2012). Yet, an exact comparison is not possible, because the statistics depend on the experiment period and temporal resolution of the validation time series.
With SMOS Tb data assimilation and when using gauge-corrected (CPCU) precipitation, the RMSDub between simulations and gridcell-scale in situ measurements (also used in the core validation of SMAP products) is 0.034 m3 m−3 for surface soil moisture at 10 reference grid cells across the United States, and also 0.034 m3 m−3 for root-zone soil moisture at the five reference grid cells with such data. Because the benefit of Tb assimilation is found to be larger when no precipitation corrections are used, we expect that SMOS (or SMAP) assimilation has a greater impact on soil moisture estimates over regions such as Africa and Asia, where both high-quality meteorological information (including precipitation gauge measurements) and in situ validation data are unavailable.
The globally averaged values of the time series standard deviation in the increments for the total soil water column and for surface soil temperature are 0.004 m3 m−3 and 0.7 K, respectively. The values are very small when averaged in time and space, because many small increments are associated with distant updates in the 3D filter (extrapolation). Yet, the corresponding mean absolute difference in soil moisture between the open loop and assimilation estimates can reach up to 50% of the temporal variability, and the energy and runoff fluxes are changed by roughly 15% relative to the temporal variability per season.
The EnKF provides global uncertainty estimates for all variables in the land surface data assimilation system. With assimilation, the globally averaged uncertainty for the analyzed surface and root-zone soil moisture is 0.02 and 0.01 m3 m−3, respectively, which is a fraction of the uncertainty without any assimilation (0.85 for global surface soil moisture and 0.74 for global root-zone soil moisture).
To summarize, SMOS Tb observations are predominantly related to surface soil moisture and temperature and vegetation conditions. The Tb data assimilation successfully (i) increases the effective vertical penetration depth through propagation of surface information to the root zone, (ii) increases the spatial and temporal coverage by interpolation and extrapolation to unobserved times and locations, and (iii) provides consistent estimates of various land surface state and flux estimates with reduced uncertainty. In future research and in the forthcoming SMAP L4_SM product, the spatial resolution of the land model within the assimilation system and therefore the resolution of the assimilation estimates will be increased to 9 km. The analysis component of this future system will thus downscale the coarser (36 km) brightness temperature observations to the finer (9 km) resolution of the modeling system.
Acknowledgments
The authors thank Yann Kerr for his assistance with the SMOS data, Mike Cosh and Tom Jackson for providing the in situ data for the SMAP core validation watersheds, Jeffrey Walker and Xiaoling Wu for providing a part of the Oznet data, Qing Liu for helping with the quality control of sparse network data, and the reviewers and Hans Lievens for suggestions to edit the paper. The study was supported by the NASA Soil Moisture Active Passive (SMAP) mission. Special thanks go to our SMAP L4_SM collaborators Randy Koster, Wade Crow, John Kimball, and Qing Liu. Computational resources were provided by the NASA High-End Computing (HEC) Program through the NASA Center for Climate Simulation (NCCS) at the Goddard Space Flight Center.
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