The European Space Agency launched the Soil Moisture Ocean Salinity (SMOS) satellite in November 2009. Using SMOS soil moisture retrievals for 2010 processed using algorithm V4.00, we evaluated SMOS retrievals by comparing them to in situ soil moisture observations for the top 5 cm at several stations in the Great Plains of the U.S. A major issue with comparing the satellite data with in situ data is that a SMOS footprint is about 40 km across and we compare to point observations. To address this issue, we chose locations in Oklahoma that have 10 to 25 different in situ observations within each SMOS footprint. The SMOS retrievals have a dry bias when compared to the average of all in situ stations in a footprint. Large differences exist between the in situ observations, even for probes only a few meters apart. Observations from different sensors within a SMOS footprint differ from each other by a larger amount than they differ from the SMOS retrieval. Removing the mean and normalizing the data bring the in situ observations into better agreement with each other and with SMOS but there are still substantial differences. Agricultural Research Service Micronet regions in Oklahoma had highly varying values of soil moisture despite being in close proximity to one another, but when averaged and compared to SMOS they had less of a bias than the other regions. Further north in the Great Plains, SMOS retrievals of top 5 cm soil moisture from descending orbits were consistently about 5% by volume wetter than ascending retrievals.
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 Soil moisture makes up only 0.01% of the total water on the planet [Prigent et al., 2005]. Soil water content is important for many reasons, such as agriculture. Soil water content also has an important influence on climate, as it determines the partitioning of energy at the surface between sensible and latent heat [Li et al., 2007; European Space Agency (ESA), 2002]. To better understand the interactions of soil moisture with the climate system, an accurate assessment of soil moisture globally must be made. Land surface models have been able to estimate the global soil moisture distribution, but are handicapped by their lack of access to reliable information on soil properties and atmospheric forcing, as well as inaccuracies in the models themselves. It is also difficult to evaluate how well the models simulate the actual soil moisture [Prigent et al., 2005]. In situ observations only cover a small fraction of the planet, as the cost of direct observation of soil moisture is very high [Vinnikov et al., 1999]. However, a satellite can orbit the entire planet daily and provide routine soil moisture measurements for every location [Kerr et al., 2001], even those that are not inhabited by humans. As in the case of the land surface models, it is difficult to evaluate the remote sensing retrievals of soil moisture. However, in locations with in situ observations it is possible to compare the two different measurements and evaluate the effectiveness of the satellite.
 Satellite sensors measure soil moisture at a large spatial resolution while in situ stations measure soil moisture at a single point [Jackson et al., 2010]. Therefore, locations can only be used as evaluation sites if there are sufficient in situ stations. It has already been shown that there is significant spatial variability of soil moisture. Entin et al.  have established a spatial autocorrelation of soil moisture of about 500 km, much greater than any regions being looked at in this study. However, they also suggested that there is a smaller scale of variation that is dominated by land surface variations. Crow and Wood  also claimed that there were differences between the coarse scale (>10 km) and the fine scale (<1 km) and attributed the fine scale variability to the effects of local variations in topography, soils, and vegetation. However, while the aforementioned studies focused on the stations themselves, here we will attempt to create a mean data set to evaluate SMOS footprints in different regions only where there are many in situ stations in a very small area.
 Satellite microwave measurements can only sample the topsoil layer, typically only a few cm. Microwave observations of soil moisture from satellite radiometers are sensitive to the effects of water on the dielectric constant of the soil, which affects the emissivity [Jackson and Schmugge, 1989]. Using satellite data in conjunction with land surface data will allow for a global data set of soil moisture to be assimilated into a model, which may allow for better prediction of precipitation over land [Reichle et al., 2004]. Here we evaluate satellite retrievals of top 5 cm soil moisture by using dense networks of in situ soil moisture observations and the Soil Moisture Ocean Salinity (SMOS) satellite. The European Space Agency launched SMOS in November 2009. According to Kerr et al. , SMOS is designed to have an error less than 0.04 m3/m3 and a spatial resolution better than 50 km. ESA  projects a resolution between 35 and 50 km. SMOS is not the first satellite to directly measure soil moisture, as other satellites such as the Advanced Microwave Scanning Radiometer (AMSR-E) on board the Aqua satellite and the Scanning Multichannel Microwave Radiometer (SMMR) have been used. AMSR-E measured soil moisture at a resolution of 60 km at a frequency of 6.92 GHz [Njoku et al., 2003] and SMMR measured at a frequency of 6.63 GHz [Reichle et al., 2004]. However, frequencies in this range (C-band) are more sensitive to errors resulting from the effects of vegetation and surface roughness, and do not retrieve signals from other than the very top cm or two of the soil. At lower frequencies (longer wavelengths), this effect is decreased, but too low a frequency will result in interference from anthropogenic radio waves. Frequencies of 1–2 GHz (L-band) are ideal for soil moisture measurements [Njoku et al., 2003]. Vinnikov et al.  explained that L-band radiometers can penetrate the vegetation canopy and that the retrievals would be primarily a function of soil moisture. SMOS is different from the other satellites, in that it operates at a frequency within this range, 1.4 GHz [Kerr et al., 2001; ESA, 2002].
 Sun synchronous satellites make both an ascending and a descending pass each day. In the case of SMOS over the central United States, descending passes occur during the evening between 00 UTC and 01 UTC and ascending passes occur in the early morning between 11 UTC and 12 UTC. This corresponds to the plan made by Kerr et al. , which called for a sun synchronous orbit and 6 A.M. ascending passes to coincide with sunrise. During the day, surface drying may create errors as the near surface layer (0–1 cm) may undergo significant drying [Njoku et al., 2003] and not be representative of the in situ soil moisture data which is measured to a depth of 5 cm. Therefore, ascending and descending passes are separated in this study to determine if there is a difference between the two.
 Several different in situ sites were used across the central United States. The high density of sites near Stillwater, Oklahoma, was beneficial as not only was there a high number of stations within a single SMOS footprint, but it also enabled an investigation of the in situ data themselves. The same is true for the two ARS Micronets. Each of the in situ data sets is described here. Table 1 provides a list of all in situ stations used, their coordinates, and their elevations. It is important to consider that the in situ soil moisture stations measure soil moisture at 5 cm depth while SMOS claims to retrieve an average of the 0–5 cm depth. Direct in situ measurements at a depth closer to the surface could prove problematic, as factors such as erosion and biological activity can expose the sensor to the air above. Other recent studies have used 5-cm data to compare to satellite observations, including Jackson et al. , Albergel et al. , and Pathe et al. .
Table 1. List of All in Situ Stations Used in This Study
Stillwater, OK Region
USCRN Stillwater, OK 5 WNW
USCRN Stillwater, OK 2 W
COSMOS SMAP OK
Little Washita Micronet Region
Little Washita Micronet (18 stations)
SCAN 2023 Little Washita, OK
Fort Cobb Micronet Region
Fort Cobb Micronet (15 stations)
USCRN Aberdeen, SD 35 WNW
SCAN 2002 Crescent Lake, MN
SCAN 2020 Mandan, ND
2.1. United States Climate Reference Network (USCRN)
 The United States Climate Reference Network (USCRN) is maintained by the National Climatic Data Center (NCDC) (http://www.ncdc.noaa.gov/crn/). The first USCRN soil moisture sensors were installed in Crossville, Tennessee, in April 2009. Each station consists of sensors placed at 5, 10, 20, 50, and 100 cm depths. At each individual depth, three sensors are located around the main tower and are only several meters apart [LeDuc et al., 2010]. The sensor used is the Stevens Hydra Probe and its calibration procedures are outlined by Seyfried et al. . The benefit to using three sensors is that soil moisture variations on a very small scale are captured as even the slightest variation in soil texture can change its water content. Also, if one of the sensors malfunctions the other two will continue to provide measurements eliminating the potential for long periods of downtime at any particular station. This study uses hourly observations of soil moisture at 5 cm depth for the 2010 calendar year. (Data for every USCRN soil moisture site are available at http://www1.ncdc.noaa.gov/pub/data/uscrn/products/soilsip01/.)
2.2. Soil Climate Analysis Network (SCAN)
 The Natural Resources Conservation Service (NRCS) of the United States Department of Agriculture (USDA) operates the SCAN network, which consists of 129 stations located in 39 states [Schaefer et al., 2007]. SCAN data have been available from the three locations used in this study, Little Washita, OK, Mandan, ND, and Crescent Lake, MN since 1996, 1997, and 1998 respectively. Like the USCRN, in this study hourly soil moisture measurements at 5 cm depth for 2010 are used. Each SCAN station has instrumentation to measure soil moisture at depths of 5, 10, 20, 50, and 100 cm depths [Njoku et al., 2003], which is identical to the USCRN. The mean station density is one station per 85,000 km2 [Jackson et al., 2010]. The sensor used is the Stevens Hydra Probe, as used for USCRN. (Data for every SCAN station are available at http://www.wcc.nrcs.usda.gov/scan/.)
2.3. Oklahoma Mesonet
 The Oklahoma Mesonet consists of over 100 sites measuring 5 cm soil moisture every 30 min. The mean density of the soil moisture network is one station per 1677 km2, which is much higher than SCAN. Soil moisture is also measured at 25, 60, and 75 cm depths but at fewer locations [Illston et al., 2008]. To remove extremes of both bare soil and fast growing vegetation, only locations with uniform, low growing vegetation were used as Mesonet station locations [McPherson et al., 2007]. The sensor used is the Campbell Scientific 229-L. It is cylinder-shaped and has a length of 60 mm and a diameter of 14 mm [Illston et al., 2008]. A ceramic matrix surrounds 32 mm of the cylinder and inside is a thermocouple and a resistor [Illston et al., 2008]. The temperature is measured by the thermocouple before and after a 21-s heat pulse is transmitted through the resistor [Illston et al., 2008]. The difference between the two measurements provides information on the soil water potential which can be translated to soil water content [McPherson et al., 2007] using an empirical relationship developed by Arya and Paris , which requires information on the particle size distribution and the bulk density of the soil, both of which are available in soil survey reports. For wet soil the temperature difference will be smaller and for dry soil the difference will be larger [McPherson et al., 2007]. Calibration of the sensor is done in a laboratory by attempting to obtain the highest and lowest values of heat dissipation. First the sensor is placed into a bag with desiccant to remove moisture to obtain the largest temperature difference to simulate the driest possible conditions. Then the sensor is placed into a beaker of distilled water and as a result is saturated, allowing the lowest possible value of dissipation to be measured simulating the wettest possible conditions [Illston et al., 2008].
2.4. Cosmic Ray Soil Moisture Observing System (COSMOS)
 The COSMOS probe measures soil moisture every hour beginning July 21, 2010. The data are different from the other sources in that the sensors are placed above ground and the soil is not disturbed. Measurements of soil moisture on a horizontal scale of about 670 m and a vertical depth between 12 cm (wet soil) and 76 cm (dry soil) are inferred by measurements of cosmic ray neutrons that are generated within the soil and emitted back to the atmosphere, where they are measured [Zreda et al., 2008]. The backscattered flux of slow neutrons is proportional to the density of hydrogen atoms. Since water is the major source of hydrogen atoms that changes with time, the neutron probe can yield a good estimate of soil moisture [Robock et al., 2000]. Benefits to this technique are that the footprint comprises a large volume rather than a single point; although the size of the area in the case of COSMOS is still much smaller than the size of the SMOS footprint. (Data are available at http://cosmos.hwr.arizona.edu/.)
2.5. Agricultural Research Service (ARS) Micronet
 The ARS operates two Micronets in southwestern Oklahoma; Little Washita and Fort Cobb. They consist of high density soil moisture measurements every 15 min at 5, 25, and 45 cm depths. For this study, 18 stations from the Little Washita Micronet and 15 stations from the Fort Cobb Micronet were used. The Little Washita Micronet was first established in the early 1990s and the Fort Cobb Micronet in 2005. Cosh et al.  have determined that the average soil moisture from all of the stations in the Micronet is a good representation of the mean soil moisture within the watershed based on results from Soil Moisture Experiment 2003 (SMEX03). The sensor used is the Stevens Hydra Probe, the same as for SCAN and USCRN. (Data from the two Micronets as well as information about the individual sites are available for download at http://ars.mesonet.org.) Because of the large number of sites, a range of coordinates and elevations was given in Table 1 rather than listing them individually for each station. A map of the region encompassing the two Micronets is shown in Figure 1. The map is divided into areas representing weights used for a type of averaging described at the end of section 3 and is referred to as a Voronoi plot.
 The SMOS satellite was launched at the end of 2009 and underwent its commissioning phase through May of 2010. During that time frame and extending into the fall of 2010 many changes were made to the algorithms used to determine soil moisture. To provide a consistent data set for calibration and validation, the 2010 data set was reprocessed with the latest version of the algorithms, which is the V4.00 data being used in this study (Expert Support Laboratories and Array Systems Computing, Release of SMOS level 2 reprocessed soil moisture products, read-me-first note, 2011, http://calvalportal.ceos.org/cvp/c/document_library/get_file?uuid=98ef88d1-c266-41d0-9a36-55a666814b88&groupId=10136). The basic mechanism by which SMOS measures soil moisture is through the relationship between microwave emissivity in the L-band (1.4 GHz) and moisture. SMOS measures the brightness temperature, which is a function of the emissivity, and therefore a function of near surface (0–5 cm depth) soil moisture. The exact retrieval methods are described by Kerr et al. . A weighting function is applied to SMOS measured brightness temperatures since they are measured at different incidence angles, which could affect the results. The values for each pixel are compared to modeled brightness temperatures and a cost function is generated which minimizes the differences between the modeled brightness temperatures and the SMOS weighted brightness temperatures. This is the main component of the soil moisture retrieval algorithm. The actual retrievals are performed on subsets of the weighted pixels, which correspond to soils with low vegetation. The SMOS field of view is not circular, as it has more of a hexagonal shape with concave sides [Kerr et al., 2001]. However, this study assumes a circular field of view with a radius of 40 km and a uniform region of influence where the SMOS value is said to be equal across the entire footprint. This is a simplification due to differences in vegetation and soil type. If two center points are within 40 km of each other, there will be overlap of the footprints. SMOS can pass over a given location on an ascending or a descending orbit. This study separates the two types of passes to see if there are any relationships between the time of the SMOS pass and the results found. With no precipitation one would expect a diurnal cycle of soil moisture with wetter soil at night and drier soil during the day because of the changing evaporative demand. Thus, it should be expected that ascending passes should have higher soil moisture values than descending passes.
 We created time series for the entire calendar year 2010 using the data sets described above. The location around Stillwater was chosen due to the large number of stations in that region. The Oklahoma Mesonet sites at Stillwater (STIL), Marena (MARE), and Perkins (PERK) were used, as well as USCRN sites Stillwater 2 W and Stillwater 5 WNW and the COSMOS SMAP OK site. Each USCRN site contains three soil moisture sensors, which we plotted individually and the COSMOS data are only available starting July 21. A Voronoi plot of the station locations is shown in Figure 2. Another map showing the close proximity of the USCRN stations, as well as the Mesonet STIL station is shown in Figure 3. The SMOS center point was chosen so that all of the in situ stations reside within the footprint meaning that each station is no more than 20 km from the center point. The haversine formula was used to calculate the distance between two points and find which points would be acceptable for use. Two SMOS points around Stillwater met the criteria and were used in this study. These two points and their respective footprints are outlined in Figure 2. The points on all the SMOS time series plots are color coded to reflect ascending and descending passes.
 For the Stillwater region we removed the annual mean soil moisture values for each individual data set to account for systematic biases (Figure 4) and normalized the data by dividing by the standard deviation of each data set. Scatterplots were created to perform a statistical analysis of the data. To assess SMOS performance, the in situ data sets were arithmetically averaged together to create a mean data set which represented the approximate in situ soil moisture of the SMOS footprint which was compared to the values retrieved by SMOS for that footprint (Figure 5). This same approach was used by Jackson et al.  in validation of AMSR-E data. Scatterplots were made for the raw data for both SMOS footprints (Figure 6). Each plot included the correlation coefficient (r), the root mean square error (RMSE), and the bias (b). Bias was calculated by taking the difference between each SMOS and the averaged in situ measurements and taking the mean. RMSE was calculated by taking the difference of each SMOS and the in situ measurements, squaring them, and then taking the mean. To show the relationship between ascending and descending points, the values of r, RMSE, and b were computed only considering times when in situ data correspond with ascending or descending passes and represent the different colors on the plots. The aforementioned techniques were also used in analyzing the second SMOS center point.
 The variability of the ARS Micronet stations in Fort Cobb, OK and Little Washita, OK was examined. For each watershed, all of the Micronet data were averaged and compared to SMOS as in Stillwater. The SMOS center point was chosen so that most, if not all, of the stations would fall into a single footprint. Time series were created for the Little Washita and Fort Cobb watersheds (Figures 7 and 8, respectively) which include a time series of all of the individual Micronet stations as well as the average of all of the stations for the respective watershed. Mesonet sites at Acme (ACME) and Apache (APAC) as well as SCAN site 2023 (Little Washita) all fall within the Little Washita Micronet and were included in the time series plot. The Mesonet site at Hinton (HINT) is within the Fort Cobb Micronet and is subsequently included in its plot. Scatterplots for the two Micronets were generated in the same manner as for Stillwater showing the same statistical variables (Figure 9). Only the Micronet data were considered for the scatterplots as the SCAN and Mesonet data were only plotted in the time series for a visual reference. Figure 9 (top) represents Little Washita and Figure 9 (bottom) represents Fort Cobb.
 The averaging scheme used to generate the mean data sets used in the scatterplots was a simple arithmetic average in which all stations were given equal weight. To determine if differences would exist if the weights were given based on the number of stations and proximity of the stations to each other, a second type of averaging was introduced. This method uses Thiessen polygons to divide a region into areas, as illustrated in Figures 1 and 2. Each area will consist of one in situ station and its areal fraction relative to the SMOS footprint will represent the weight of that station used in the averaging. If at a particular time, the station has an undefined value, the arithmetic mean of all of the stations is substituted for that particular time. Using this scheme, differences were minimal when compared to the arithmetic averaging. The mean difference for Stillwater footprint #1 was largest with an annual mean 0.02 m3/m3 increase in soil moisture. Stillwater footprint #2 had a mean 0.01 m3/m3 decrease in soil moisture for the year. Both Micronets had a 0.01 m3/m3 increase in soil moisture when the varying weights were applied. Because these differences were not substantial, the scatterplots were not recreated with these data, as the results would remain the same. For a visual representation of this method the weighted means were added to the Micronet time series (Figures 7 and 8).
 Just looking at soil moisture in Oklahoma is not sufficient for a full evaluation. We also examined soil moisture stations located farther north. Because there are only a limited number of in situ stations, the SMOS evaluation is not complete in this region, but the results reveal certain patterns within the SMOS retrievals themselves. We also examined USCRN site Aberdeen 35 WNW in South Dakota, SCAN site 2002: Crescent Lake, Minnesota, and SCAN site 2020: Mandan, North Dakota. For each station a time series was created for the 5-cm soil moisture in situ data as well as that for the closest SMOS point (Figure 10 for Aberdeen 35 WNW, other stations not shown). Scatterplots were also created for each of the stations and show the same information as those created for Stillwater (Figure 11 for Aberdeen 35 WNW, other stations not shown).
 To assess the spatial variability further, semi-variograms along with correlation lag plots were created. The semi-variograms were created using the method described by Liu et al.  and provide information on the relationship of soil moisture measurements at close distances. The distance between each pair of the three USCRN sensors at one station was assumed to be 5 m. The bins were done at 5 km intervals except in the case of Stillwater where the first averaged value represents the mean of the 5 m data only, which represents the individual USCRN sensors at the two stations. This was done to analyze the nugget effect, since this distance is essentially equal to zero when compared to the other distances used, which are on the order of 104 m. The points at (0,0) on the semi-variograms and (0,1) on the correlation lag plots were removed since it is unnecessary to account for the relationship of one station with itself. The semi-variograms and correlation lag plots are shown in Figure 12 with the semi-variograms on the left and the corresponding correlation lag plot to the right of its respective semi-variogram.
 The time series of the in situ stations around Stillwater, seen in Figure 4, shows large differences among the soil moisture data from the different stations. It appears that the Oklahoma Mesonet sites have higher mean soil moisture than the other stations with yearly means for STIL, MARE, and PERK of 0.42 m3/m3, 0.33 m3/m3, and 0.34 m3/m3 respectively. The differences between the in situ stations are as large as the differences between the SMOS retrieval and each in situ station. Removing the mean (Figure 4, bottom) brings the data into closer agreement but large differences still exist, particularly during rapid upward increases in soil moisture after precipitation. This can be attributed to both the high spatial variability of precipitation as well as differences in soil properties at each in situ station. For example, sensor 1 from USCRN 5 WNW shows a strong upward increase due to precipitation in the beginning of the year since its yearly mean is so low (0.19 m3/m3) compared to other sensors. However, the other sensors do not have values this high. In fact the Mesonet sites have much smaller values because their means were so high. The standard deviation of the USCRN sensors is higher than the others with values ranging between 0.09 m3/m3 and 0.12 m3/m3. The range of the standard deviation for the Mesonet sensors is between 0.05 m3/m3 and 0.07 m3/m3. COSMOS has the smallest standard deviation of 0.04 m3/m3. When the data are normalized by dividing each mean removed time series by its respective standard deviation (not shown) it appears the variations are in better agreement, but the values themselves are still different and no closer in proximity to just using mean-removed values. The total RMSE (ascending and descending combined) for SMOS center point 1 and SMOS center point 2 is 0.12 m3/m3 and 0.13 m3/m3 respectively. Upon removing the mean of the data, the RMSE values both reduce to 0.06 m3/m3. Normalizing results in a RMSE of 0.07 m3/m3 for the two points.
 The average of all the in situ data is plotted along with the two SMOS footprints in Figure 5. The SMOS footprints are similar but do show some differences such as the case described above. For the most part, the mean of the two SMOS center points falls below the mean of all of the in situ points, illustrating the overall negative bias. The scatterplots in Figure 6 reveal that the two footprints offer similar statistics, which are expected since there is a large amount of overlap. Both show good correlation between the in situ and the SMOS but show a strong negative bias. For these points there is no difference between the ascending and descending passes as biases are still between –0.09 m3/m3 and −0.11 m3/m3.
 The Oklahoma Micronet data for the Little Washita and Fort Cobb Micronets were plotted in Figures 7 and 8, respectively. Both show strong variability between the individual stations consistent with the results from Stillwater. The mean spread of the soil moisture values from the Micronets were 0.23 m3/m3 and 0.24 m3/m3 for Little Washita and Fort Cobb respectively. The spread is defined as the difference between the maximum observed soil moisture value and the minimum soil moisture value at the same time. With such a large spread it is difficult to compare to SMOS observations. The maximum spread of the Little Washita Micronet was 0.50 m3/m3, which is extremely large. The lowest spread value computed for both Micronets was 0.11 m3/m3, which is larger than the negative SMOS biases measured at Stillwater. When both Micronets were averaged into one time series the mean Micronet values became 0.14 m3/m3 and 0.15 m3/m3 for Little Washita and Fort Cobb respectively. The Mesonet sites ACME and APAC, within the Little Washita region, registered mean values of soil moisture of 0.33 m3/m3 and 0.35 m3/m3 respectively. The nearby SCAN site had a mean value of soil moisture of 0.31 m3/m3. The HINT Mesonet site near Fort Cobb had a mean soil moisture of 0.32 m3/m3. The Mesonet data and SCAN data were not included in the SMOS comparison because their soil moisture values were much higher than those from the Micronets. This can be seen visually in Figures 7 and 8. As is apparent in Figure 9, there was no bias for Little Washita, which was inconsistent with the results found near Stillwater. At Fort Cobb there was a bias of –0.04 m3/m3, which is not as pronounced as for Stillwater. The RMSE for the watersheds were 0.05 m3/m3 and 0.07 m3/m3 for Little Washita and Fort Cobb respectively and not within 0.04 m3/m3 as desired by SMOS.
 It is evident from Figure 10 that at USCRN site Aberdeen 35 WNW, there are oscillations between ascending and descending passes with higher soil moisture values occurring for descending passes and lower values for ascending passes. Figure 11 shows the scatterplot for the Aberdeen data. The correlations for ascending and descending passes are almost equal (about 0.70), but when combined decrease to 0.63. The negative bias for the ascending passes is larger than for the descending passes. This contradicts the supposition that soil moisture should be at its driest in the late afternoon as SMOS registers the opposite. The same results were seen for the data at two other sites, SCAN 2020 Crescent Lake and SCAN 2092 Mandan. SCAN 2020 recorded a descending bias of −0.08 m3/m3 and an ascending bias of −0.11 m3/m3. SCAN 2092 had a descending bias of −0.20 m3/m3 and an ascending bias of −0.26 m3/m3. For all of the northern sites, an additional SMOS center point was chosen and similar results were found indicating that these findings are not the result of an isolated error. These results are because of radio frequency interference from the North Warning System radars across northern Canada (formerly called the Distance Early Warning (DEW) Line), which preferentially affect the ascending retrievals because of the SMOS antenna pattern (Y. Kerr, personal communication, 2011). The radar emissions raise the brightness temperature, artificially lowering the retrieved soil moisture. There is no seasonal cycle of the difference between the ascending and descending retrievals, as the oscillations appear to occur throughout the year, further suggesting the above hypothesis is correct.
 The semi-variograms in Figure 12 all show a constant sill which is reached very quickly. For the two Micronet regions, the sill is nearly constant at every distance, which shows that there is little relationship between these points even at such close distances. A nugget effect or range cannot be seen at either Micronet region, perhaps as a result of there being no data available to diagnose them. Based on this alone it appears as if there is no spatial relationship with the Micronet data. However, correlation plots show correlations generally between 0.5 and 0.9 for both Micronets. While this is not perfect it shows that there is at least some spatial relationship between the values. That the mean line is nearly constant shows that the relationship does not depend on distance at such a close range, so theoretically the relationship between two stations 10 km apart would be the same as two stations 30 km apart. Because the data are related in this way, it was valid to use them for SMOS comparisons. Because data are available from individual USCRN sensors it is possible to analyze the semi-variance at near zero distance. Intuitively this value should be near zero, and in fact it is lower than the sill value for Stillwater. When connected to the mean bins for Stillwater, a range is seen in the first few km, which is consistent with fine scale variability described by Crow and Wood . Beyond this range, the pattern is similar to the two Micronets as the semi-variograms and correlation lag plots remain constant showing that at this scale the relationship between soil moisture measurements has little dependence on distance.
 The large discrepancy that was found with the in situ observations presents a major challenge in the evaluation of SMOS. Large differences are due to the known spatial variability of soil moisture, which is influenced by soil type, vegetation, and precipitation, as well as the fact that different instruments and measuring techniques are used. For example, the Little Washita Micronet has soil types that range from a fine sand to a silty loam and SCAN site 2023, which is within that region, has a silty clay soil. Because soil type affects how water infiltrates the soil surface, it is expected that there would be different values of soil moisture at each station. Although the individual values are different, semi-variogram analysis shows that there is almost a constant relationship between the stations that neither improves nor degrades with increasing distance, meaning that although the actual values may the different, the trends are similar. Previous work by Crow and Wood  and Entin et al.  describe two scales of soil moisture, but it is possible there could be a third, intermediate scale where the relationship between soil moisture and distance is constant. Studies that attempt to assimilate SMOS data into numerical weather models will face uncertainty in that it will be difficult to assess whether or not the SMOS data being put into the model are accurate enough. It also must be taken into account that SMOS evaluation is not possible when there is snow cover. In the case of Stillwater, according to National Operational Hydrological Remote Sensing Center snow cover analyses, most of Oklahoma was covered in snow during January and February 2010. Although according to Table 2, the monthly average departures between SMOS and in situ were among the highest, there was most likely error on both sides and not representative of the SMOS evaluation for the rest of the year. In places further north, snow cover is more persistent leading to an even greater time period without proper evaluation. For the USCRN site in Aberdeen, in situ data are missing for January, February, March, and December (Figure 7).
Table 2. Monthly Averaged Values for 2010 of Top 5-cm Soil Moisture (m3/m3) Derived From the in Situ Mean and the Two SMOS Footprints Around Stillwater (Figure 2)a
In Situ Mean
The averaged monthly SMOS biases (as compared to in-situ mean) are also given for each footprint. SMOS difference is the difference between the two SMOS retrievals (SMOS 1 minus SMOS 2).
 One important consideration in these comparisons is that the SMOS footprint covers a large area. If there is a rainfall event that produces wet soil in a part of the footprint that has no in situ stations, large differences could result. As expected, the soil moisture both from in situ and SMOS appears higher in the winter and early spring than in the middle of the summer because evaporative forcing is higher in the summer. This can be seen in more detail in Table 2. SMOS recorded its highest value of 0.59 m3/m3 at two times, 12 UTC March 25 and 12 UTC April 2, both from center point #1. It was confirmed through looking at archived Next Generation Radar (NEXRAD) images available from NCDC (http://www4.ncdc.noaa.gov/cgi-win/wwcgi.dll?WWNEXRAD∼Images2), that precipitation was falling at the times of the two measurements. However, the second footprint retrieved observations of 0.45 m3/m3 on the March 25 and 0.41 m3/m3 on April 2, which were substantially smaller than that of the first footprint. Based on the radar data it appeared that the rainfall was widespread over the two footprints. The second footprint shows some dry observations in early April that were not present in the first footprint and explains the large difference between the two monthly averages, as seen in Table 2. In the case of the extreme values of SMOS, it is uncertain as to whether or not the satellite was recording extra water that did not infiltrate the soil, making the value higher than it otherwise would be. Based on the Figure 4 precipitation plot, there were times during the year, particularly on May 19 and June 14 where precipitation was higher than it was on March 25 and April 2. However, SMOS provided undefined values for those days, making it impossible to determine the relationship with the precipitation. It should also be noted that precipitation has a high spatial variability and will not be uniform over an area even as small as that in Figure 3. Therefore, it will be difficult to determine the exact relationship between SMOS and precipitation, but one would intuitively expect that precipitation should lead to an increase in SMOS values.
 The reduction in the RMSE from the two footprints near Stillwater that resulted from removing the means shows that it might be better to evaluate SMOS after removing all of the station biases as well as the bias of the SMOS point. This shows that SMOS is better at observing trends in soil moisture rather than instantaneous values. However the RMSE is still greater than the required accuracy of 0.04 m3/m3. More work will need to be done investigating the sites to the north and the reasoning for the oscillations between the ascending and descending passes.
 The radio frequency interference we found in the northern part of our domain will affect broad regions of the world, and with a larger amplitude as other regions have even larger surface microwave emissions. This further adds to the errors in SMOS retrievals, but if the emissions are relatively constant, perhaps useful corrections can be made.
 Although the negative biases for SCAN 2020 were much larger than the other sites, it cannot be determined whether or not this is from SMOS or the result of an over-estimation of in situ soil moisture. This is another example of why it is difficult to evaluate SMOS.
 At present time SMOS evaluation is difficult, due to the lack of uniform soil moisture measurements within a single footprint. Differences were apparent between the three sensors at the USCRN stations that are only several meters apart as well as within the high density Micronet networks.
 To perform a better evaluation, additional monitoring sites need to be established at other locations and soil moisture data must be made available in an effort to assist with evaluation and calibration of SMOS and eventually the Soil Moisture Active Passive (SMAP) mission, which will be launched by NASA in 2014. Campaigns such as the Global Soil Moisture Data Bank [Robock et al., 2000] and the International Soil Moisture Network [Dorigo et al., 2011] have already made this possible.
 With the present set of in situ data it can be concluded that the reprocessed SMOS soil moisture data have a dry bias, which places the data below their specified accuracy range. In all but one of the analyses, SMOS came back with a dry bias below that range. Removing the mean and normalizing the data to remove the bias still results in high RMSE values relative to the desired error range. Further studies will need to be conducted at additional sites to see if this holds.
 This work is supported by NASA grant NNX09AJ99G and is conducted as part of the SMOS Validation and Retrieval Team activities. We thank Yann Kerr for the reprocessed SMOS data and for valuable comments on the manuscript, Michael Palecki for the USCRN data, Marek Zreda for the COSMOS data, and Eric Wood for providing us with the reprocessed SMOS data for 2010.