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Enhanced Resolution

warning

Soil Water Content is no longer sold at 20 m and 100 m resolution. Active contracts remain fully supported through their remaining terms, and the core infrastructure will officially sunset in April 2028. Upon renewal, please contact your Account Executive to transition to our 1000 m product variant or explore other suitable alternatives for your specific use case.

Soil Water Content 100 m​

Product Specifications​

Table 1: SWC 100 m product specification

Data ResourceSWC 100 m L bandSWC 100 m C bandSWC 100 m X band
Source IDSWC-SMAP-L_V2.0_100SWC-AMSR2-C_V2.0_100SWC-AMSR2-X_V2.0_100
Satellites UsedAMSR-2, SMAP, Sentinel-2AMSR-2, Sentinel-2AMSR-2, Sentinel-2
BandL bandC bandX band
Version2.02.02.0
Unitm³/m³m³/m³m³/m³
Sensing Depth~5 cm~2 cm~1 cm
Pixel Size100x100 m100x100 m100x100 m
Temporal Resolution0° latitude: 137 to 183 observations per year

40° latitude: 183 to 228 observations per year
0° latitude: 205 to 228 observations per year

40° latitude: 274 to 292 observations per year
0° latitude: 205 to 228 observations per year

40° latitude: 274 to 292 observations per year
Overpass Time06:00 local solar time01:30 local solar time01:30 local solar time
Geographical CoverageGlobalGlobalGlobal
Data Availability2017-07-01 - Present

Data Gaps:
2019-06-19 to 2019-07-24
2022-08-05 to 2022-09-24
2022-11-16 to 2022-11-18
2017-07-01 - Present2017-07-01 - Present
NRT latency (p90)72 hours48 hours48 hours
Archive latencyWithin 30 days after creating a subscriptionWithin 30 days after creating a subscriptionWithin 30 days after creating a subscription

The sensing depth described in the table is an estimation of the average condition. Several studies (For example, Schmugge et al., 1986; Wang et al., 1987; Owe et al., 1998) have shown that microwave-based soil water content penetration depth depends on the soil water content conditions and frequency. At 1.41 GHz the penetration depth varies from approximately 10 cm to 1 m for soil conditions ranging from saturated to dry, whereas at 10.7 GHz the penetration depth varies from less than a few mm to a little over 2 cm for similar conditions. Thus, the drier the soil, the deeper the sampling depth.

Asset Properties​

Each SWC 100 m observation is delivered as a SWC data asset (*swc.tif) with metadata provided in a separate quality flag asset (*swc-qf.tif).

Table 2: Asset properties of SWC 100 m data resources

Asset NameBand NameUnitTypeTypical RangeNo Data ValueScaleFormat
swcBand 1m3/m3UINT160 - 1655350.001GeoTIFF
swcBand 2m3/m3UINT160 - 1655350.001GeoTIFF
swc-qfBand 1unitlessUINT16NA01GeoTIFF

Enhancements Using Optical Data​

The microwave observations are further downscaled to a spatial resolution of 100 m based on the Normalized Difference Shortwave Infrared (NDSWIR) index. This index is constructed from Near-Infrared (NIR) and Shortwave Infrared (SWIR) bands of Sentinel-2, namely B08 (842 nm) and B11 (1610 nm).

Several studies (Lobell & Asner 2002, Fensholt and Sandholt 2003, Sadeghi et al. 2017, Yue et al. 2019) found that soil and plant water content significantly affect the reflection in the SWIR part of the spectrum. The NIR reflectance is influenced by the internal structure and dry matter content of leaves, but not by water content. By combining SWIR, which responds to water content, with NIR reflectance, we can more accurately retrieve water content from the reflectance data (Gao 1996, Ceccato et al. 2001).

Planet produces a daily NDSWIR composite using a backward Gaussian weighted distribution. This composite integrates into the downscaling framework by attributing the weight of a brightness temperature to each pixel within the footprint. The output format remains similar to that of the downscaling algorithm without NDSWIR input.

The Sentinel-2 data is extracted from L2A - Bottom of the atmosphere (BOA) - reflectance in the Sentinel-2 dataset documentation.

Input Data​

Table 3: List of inputs for SWC 100 m production

ProductDescription
Brightness Temperature L bandSoil Moisture Active Passive (SMAP) Level-1B Radiometer Half-Orbit Time-Ordered L band Brightness Temperatures, Version 5 (downloaded from NSIDC in HDF5 format). This Level-1B product provides calibrated estimates of time-ordered geolocated brightness temperatures at 1.41 GHz with a footprint size of 39x47 km. SMAP L band brightness temperatures are referenced to the Earth's surface with undesired and erroneous radiometric sources removed. Data has been available since April 2015 with a latency of 12 hours. Detailed information is available here.
Brightness Temperature X bandAdvanced Microwave Scanning Radiometer for EOS (AMSR-E) and Advanced Microwave Scanning Radiometer 2 (AMSR-2) Level-1B Radiometer X band Brightness Temperatures (downloaded from JAXA G-portal in HDF5 format). This Level-1B product provides calibrated estimates of geolocated brightness temperatures at 10.7 GHz with a footprint size of 24x42 km. Data has been available from July 2002 to October 2011 (AMSR-E) and from June 2012 (AMSR-2) up to now with a latency of 12 hours. Detailed information is available here
Brightness Temperature C bandAMSR-E and AMSR-2 Level-1B Radiometer C band Brightness Temperatures (downloaded from JAXA G-portal in HDF5 format). This Level-1B product provides calibrated estimates of geolocated brightness temperatures at 6.9 GHz with a footprint size of 35x62 km. Data has been available from July 2002 to October 2011 (AMSR-E) and from June 2012 (AMSR-2) up to now with a latency of 12 hours. Detailed information is available here.
Brightness Temperature Ka bandAMSR-E and AMSR-2 Level-1B Radiometer Ka band Brightness Temperatures (downloaded from JAXA G-portal in HDF5 format). This Level-1B product provides calibrated estimates of geolocated brightness temperatures at 36.5 GHz with a footprint size of 7x12 km. Data has been available from July 2002 to October 2011 (AMSR-E) and from June 2012 (AMSR-2) up to now with a latency of 12 hours. Detailed information is available here.
Brightness Temperature W bandAMSR-E and AMSR-2 Level-1B Radiometer W band Brightness Temperatures (downloaded from JAXA G-portal in HDF5 format). This Level-1B product provides calibrated estimates of geolocated brightness temperatures at 89 GHz with a footprint size of 3x5 km. Data has been available from July 2002 to October 2011 (AMSR-E) and from June 2012 (AMSR-2) up to now with a latency of 12 hours. Detailed information is available here.
Reflectances SWIR and NIRSentinel-2 Level-2A reflectance data for two bands: SWIR (shortwave infrared around 1610 nm) and NIR (near infrared around 842 nm).
Digital Elevation ModelDigital elevation model (DEM) static map resampled at 100 m based on the Copernicus DEM GLO-90 product covering the full global landmass of the time frame of data acquisition (2011-2015). Detailed information is available in the link.
Land Cover MapCustom global land classification including permanent water bodies based on the Copernicus Global Surface Water Bodies product from PROBA-V. Detailed information is available here
Soil MapSoil property maps resampled at 100 m based on the SoilGrids product. SoilGrids was funded by the core funding of ISRIC with additional support from the EUH2020 CIRCASA project. Detailed information is available here,

Metadata​

Quality flag assets (*swc-qf.tif) provide metadata for each pixel using bitwise flags. Critical flags indicate unreliable data, with corresponding pixels in band 1 of the SWC asset (*swc.tif) set to the no data value. The replaced SWC value can be found in band 2 of the SWC asset. Non-critical flags indicate that the data can be used with caution, taking into account the flag description.

Critical and non-critical flags are described in the tables below. For more information on how to access the quality flag asset, check out subscribing to planetary variables.

Table 4: Non-critical flags

BitFlag layerDescription
1Dense vegetationThe retrieved soil water content is less reliable over dense vegetation cover.
2Low soil water contentThe retrieved soil water content is lower than the estimated wilting point.
3High soil water contentThe retrieved soil water content is higher than the estimated porosity.
4Possible severe precipitationPart of the footprints touch an area flagged as severe precipitation.
5Possible RFIFootprints are contaminated for less than 25% with Radio Frequency Interference (RFI). RFI occurs when human-made transmitters emit in the same frequencies and thus disrupt the radiometer measurements of the natural microwave emission.
7Possible frozen soilThe soil may be frozen. These are pixels with a soil temperature between -10°C and 0°C.

Table 5: Critical flags

BitFlag layerDescription
6Statistical outlierThe underlying footprint is considered a statistical outlier.
8Frozen soilThe soil is frozen. Pixels with a soil temperature below -10°C. A conservative value of -10°C was chosen to avoid masking valid data.
9Severe precipitationSevere precipitation is detected.
10Vegetation too denseThe vegetation cover is too dense for the algorithm to reliably retrieve soil water content.
11No overpassThe satellite did not pass over.
12RFIFootprints are contaminated for more than 25% with Radio Frequency Interference (RFI). RFI occurs when human-made transmitters emit in the same frequencies and thus disrupt the radiometer measurements of the natural microwave emission.
13Instrumental flawsUnrealistic values due to instrumental flaws. If the brightness temperature at 36.5 GHz V produces values either over 400K or under 0.9 * the water temperature, the data is considered as unrealistic and is removed.
14Out of valid rangeSoil water content values are outside the valid range, meaning under 0 m3/m3 or above 1 m3/m3.
15Open waterSoil water content is not defined over water.
16Brightness temperature residuals too highThe LPRM model could not find a soil water content value that is consistent with all provided input data.

Figure 1: An example of two quality flags for a region around Nantes, France. The image shows critical flags 'open water' and 'no overpass' overlaid on SWC 100 m.

The following Python script converts a quality flag pixel value into a list of corresponding quality flags. Note that one pixel may have multiple flags applied to it.

# swc_quality_flags.py

import argparse

SWC_QUALITY_FLAGS = {
1: "Dense vegetation",
2: "Low soil water content",
3: "High soil water content",
4: "Possible severe precipitation",
5: "Possible RFI",
6: "Statistical outlier (critical flag)",
7: "Possible frozen soil",
8: "Frozen Soil (critical flag)",
9: "Severe precipitation (critical flag)",
10: "Vegetation too dense (critical flag)",
11: "No overpass (critical flag)",
12: "RFI (critical flag)",
13: "Instrumental flaws (critical flag)",
14: "Out of valid range (critical flag)",
15: "Open water (critical flag)",
16: "Brightness temperature residuals too high (critical flag)",
}


def convert_to_quality_flags(decimal_value: int) -> list[str]:
binary_string = format(decimal_value, "016b")
reversed_binary_string = binary_string[::-1]
return [
f"{i}. {SWC_QUALITY_FLAGS.get(i, 'Unused flag')}"
for i, bit in enumerate(reversed_binary_string, start=1) if bit == "1"
]


if __name__ == "__main__":
parser = argparse.ArgumentParser(description="Convert a decimal value to quality flags.")
parser.add_argument("decimal_value", type=int, help="The decimal value to convert.")
args = parser.parse_args()

flags = convert_to_quality_flags(args.decimal_value)
print(*flags, sep="\n")

that you can call as follows, using value 32770 as example:

> python swc_quality_flags.py 32770
2. Low soil water content
16. Brightness temperature residuals too high (critical flag)

Other Limitations​

  • Cloud cover hinders the optical observations by Sentinel-2 that are used for the SWC 100 m products. The downscaling can therefore only be updated when we obtain a cloud-free observation and the SWC data may suddenly increase or decrease after a long spell of no observations.

Frequently Asked Questions​

What is the difference between the SWC 20 m, 100 m, and 1000 m products?​

Our SWC 1000 m product is based on our patented disaggregation method where we make optimum use of the overlapping satellite footprints to refine the resolution from 36 km to 1 km. The SWC 100 m product also uses the NIR and SWIR band from Sentinel-2 to add more spatial constraints to our disaggregation method.

Why does the SWC 1000 m product show a higher correlation with in-situ measurements than the SWC 100 m product?​

Sometimes, customers compare our SWC products with in-situ measurements and find that the SWC 1000 m products perform better than the SWC 100 m products. This can be explained by the method used to enhance the spatial resolution. The SWC 1000 m product uses passive microwave observations, and has a temporal resolution of about 2 days, depending on the microwave band used and the latitude.

As a result, the SWC 1000 m product sees a lot of the temporal variations in SWC which are also caught by the in-situ sensor. For the enhanced-resolution products, we combine the passive microwave observations with infrared observations from the Sentinel-2 satellite. The infrared observations have a repeat cycle of about 5 days, depending on the latitude, but they cannot be made on cloudy days. The infrared data tell us how the soil water content is spatially divided within the coarser SWC 1000 m product and thus can accurately tell us which fields are relatively wet or dry, compared to the environment. However, the lower temporal resolution of the infrared data can cause the correlation coefficient to drop compared to the SWC 1000 m product. The enhanced-resolution product does get updated every time a new passive microwave observation comes in, but the temporal changes that result from the infrequent infrared observations can cause a degradation in the correlation.

Therefore, when a customer is interested mostly in the temporal changes, often the 1000 m products are the best choice. When they are interested in the spatial variations, the enhanced-resolution product can tell which areas are relatively dry or wet, compared to the environment.

Soil Water Content 20 m​

Product Specifications​

Table 6: SWC 20 m product specification

Data ResourceSWC 20 m
Source IDSWC-field_V1.0_20
Satellites UsedAMSR-2, AMSR-E, SMAP, Sentinel-2
BandL, C and X-band
Version1.0
Unitm³/m³
Sensing Depth~5 cm
Pixel Size20x20 m
Temporal Resolution267-364 observations/year
Overpass Time06:00 local solar time
Geographical CoverageGlobal
Data Availability2018-01-01 - Present

Data Gaps:
2019-06-19 to 2019-07-24
2022-08-05 to 2022-09-24
2022-11-16 to 2022-11-18

Asset Properties​

SWC 20 m is field-based: each observation is delivered as a single-band asset with metadata embedded in the GeoTIFF.

Table 7: Asset properties of SWC 20 m data resources

Asset NameBand NameUnitTypeTypical RangeNo Data ValueScaleFormat
swcBand 1m3/m3UINT160 - 1655350.001GeoTIFF

Input Data​

Table 8: List of inputs for SWC 20 m production

ProductDescription
Brightness Temperature L bandSoil Moisture Active Passive (SMAP) Level-1B Radiometer Half-Orbit Time-Ordered L band Brightness Temperatures, Version 5 (downloaded from NSIDC in HDF5 format). This Level-1B product provides calibrated estimates of time-ordered geolocated brightness temperatures at 1.41 GHz with a footprint size of 39x47 km. SMAP L band brightness temperatures are referenced to the Earth's surface with undesired and erroneous radiometric sources removed. Data has been available since April 2015 with a latency of 12 hours. Detailed information is available here.
Brightness Temperature X bandAdvanced Microwave Scanning Radiometer for EOS (AMSR-E) and Advanced Microwave Scanning Radiometer 2 (AMSR-2) Level-1B Radiometer X band Brightness Temperatures (downloaded from JAXA G-portal in HDF5 format). This Level-1B product provides calibrated estimates of geolocated brightness temperatures at 10.7 GHz with a footprint size of 24x42 km. Data has been available from July 2002 to October 2011 (AMSR-E) and from June 2012 (AMSR-2) up to now with a latency of 12 hours. Detailed information is available here
Brightness Temperature C bandAMSR-E and AMSR-2 Level-1B Radiometer C band Brightness Temperatures (downloaded from JAXA G-portal in HDF5 format). This Level-1B product provides calibrated estimates of geolocated brightness temperatures at 6.9 GHz with a footprint size of 35x62 km. Data has been available from July 2002 to October 2011 (AMSR-E) and from June 2012 (AMSR-2) up to now with a latency of 12 hours. Detailed information is available here.
Brightness Temperature Ka bandAMSR-E and AMSR-2 Level-1B Radiometer Ka band Brightness Temperatures (downloaded from JAXA G-portal in HDF5 format). This Level-1B product provides calibrated estimates of geolocated brightness temperatures at 36.5 GHz with a footprint size of 7x12 km. Data has been available from July 2002 to October 2011 (AMSR-E) and from June 2012 (AMSR-2) up to now with a latency of 12 hours. Detailed information is available here.
Brightness Temperature W bandAMSR-E and AMSR-2 Level-1B Radiometer W band Brightness Temperatures (downloaded from JAXA G-portal in HDF5 format). This Level-1B product provides calibrated estimates of geolocated brightness temperatures at 89 GHz with a footprint size of 3x5 km. Data has been available from July 2002 to October 2011 (AMSR-E) and from June 2012 (AMSR-2) up to now with a latency of 12 hours. Detailed information is available here.
Reflectances SWIR and NIRSentinel-2 Level-2A reflectance data for two bands: SWIR (shortwave infrared around 1610 nm) and NIR (near infrared around 842 nm).
Digital Elevation ModelDigital elevation model (DEM) static map resampled at 100 m based on the Copernicus DEM GLO-90 product covering the full global landmass of the time frame of data acquisition (2011-2015). Detailed information is available in the link.
Land Cover MapCustom global land classification including permanent water bodies based on the Copernicus Global Surface Water Bodies product from PROBA-V. Detailed information is available here
Soil MapSoil property maps resampled at 100 m based on the SoilGrids product. SoilGrids was funded by the core funding of ISRIC with additional support from the EUH2020 CIRCASA project. Detailed information is available here,

Metadata​

Metadata embedded in the GeoTIFF contains information about the quality of the observation. For example:

Table 9: Metadata fields of SWC 20 m data resources

FieldTypeDescriptionExample
PRODUCT_VERSIONStringVersion identifier for the product specificationv1
SOFTWARE_VERSIONStringVersion of the fbsl software that generated the output0.4.1
INPUT_ASSETSStringComma-separated list of input data sources usedNDSWIR_STATS,NDSWIR_RASTER,KA_V_DESC_STATS
LAST_NDSWIR_DATEString (ISO date)Date of the last NDSWIR (Sentinel-2) observation with full coverage2024-01-19
LAST_NDSWIR_COVString (fraction)Coverage fraction of the last NDSWIR observation used0.85 (= 85% coverage)
QUALITYStringOverall quality assessment: HIGH if valid coverage > 80%, otherwise LOWHIGH or LOW
FUSIONStringWhether L-band fusion was appliedYES or NO
DIVERGENCE_COVString (fraction)Fraction of pixels where LPRM algorithm did not converge0.05 (= 5% divergence)
QA_MDPI_LT_0_0001String (fraction)Fraction of pixels with Modified Dual Polarization Index < 0.00010.12 (= 12% of pixels)
QA_NO_COVERAGEString (fraction)Fraction of pixels with no microwave coverage0.0 (= 0% missing)
QA_FREEZINGString (fraction)Fraction of pixels flagged as freezing conditions0.0 (= 0% frozen)