The combined measurement enables global observations of the land every 2–3 days at 30 meter (m) spatial resolution. The HLSS30 and HLSL30 products are gridded to the same resolution and Military Grid Reference System (MGRS) tiling and are “stackable” for time series analysis.
Advantages of HLS


In this example of a swath product, the filename HLS.S30.T60HTE.2022103T222539.v2.0.B01.tif indicates:
The HLS tiling system is identical to the one used for Sentinel-2. The tiles’ dimensions are 109.8 km squares with an overlap of 4,900 m on each side. The system is aligned with the Military Grid Reference System (MGRS), and its naming convention is derived from the UTM (Universal Transverse Mercator) system. The UTM system divides the Earth’s surface into 60 vertical zones. Each UTM zone has a vertical width of 6° of longitude and horizontal width of 8° of latitude, as shown in the map below. Each UTM zone is subdivided into MGRS 110 x 110 km zones.
HLS uses a processing chain involving several separate radiometric and geometric adjustments, with a goal of eliminating differences in retrieved surface reflectance arising solely from differences in instrumentation.
Input data products from Landsat 8/9 (Collection 2 Level 1T top-of-atmosphere reflectance or top-of-atmosphere apparent temperature) and Sentinel-2 (L1C top-of-atmosphere reflectance) are ingested for HLS processing.
A series of radiometric and geometric corrections are applied to convert data to surface reflectance, adjust for BRDF differences, and adjust for spectral bandpass differences.
Three types of products are then generated:
1. S10 products – atmospherically corrected Sentinel-2 images in their native resolution and geometry;
The harmonized products
2. HLSS30
3. HLSL30
These products have been radiometrically harmonized to the maximum extent and then gridded to a common 30-meter UTM basis using the Sentinel-2 tile system.
Note: that S10 products are not normally archived. The S30 and L30 products are resampled as needed to a common 30-meter resolution UTM projection and tiled using the Sentinel-2 Military Grid Reference System (MGRS) UTM grid.
LP DAAC distributes both the L30 and S30 products:
S30: MSI harmonized surface reflectance resampled to 30 m into the Sentinel-2 tiling system and adjusted to Landsat 8/9 spectral response function.
L30: OLI harmonized surface reflectance and Top-of-Atmosphere (TOA) brightness temperature resampled to 30 m into the Sentinel-2 tiling system.
| Data Source | HLS Start Date |
|---|---|
| Landsat-8 | 2013-04-11 |
| Sentinel-2A | 2015-11-30 |
| Sentinel-2B | 2017-07-05 |
| Landsat-9 | 2021-10-31 |
| Sentinal-2C | 2024-09-05 |
| HLS Band Code Name L30 | HLS Band Code Name S30 | OLI Band Number | MSI Band Number | Wavelength (micrometers) | Midpoint Wavelength | Band |
|---|---|---|---|---|---|---|
| band01 | B01 | 1 | 1 | 0.43 – 0.45 | 0.44 | Coastal Aerosol |
| band02 | B02 | 2 | 2 | 0.45 – 0.51 | 0.48 | Blue |
| band03 | B03 | 3 | 3 | 0.53 – 0.59 | 0.56 | Green |
| band04 | B04 | 4 | 4 | 0.64 – 0.67 | 0.655 | Red |
| - | B05 | - | 5 | 0.69 – 0.71 | 0.7 | Red-Edge 1 |
| - | B06 | - | 6 | 0.73 – 0.75 | 0.74 | Red-Edge 2 |
| - | B07 | - | 7 | 0.77 – 0.79 | 0.79 | Red-Edge 3 |
| - | B08 | - | 8 | 0.78 – 0.88 | 0.83 | NIR Broad |
| band05 | B8A | 5 | 8A | 0.85 – 0.88 | 0.865 | NIR Narrow |
| band06 | B11 | 6 | 11 | 1.57 – 1.65 | 1.61 | SWIR 1 |
| band07 | B12 | 7 | 12 | 2.11 – 2.29 | 2.2 | SWIR 2 |
| - | B09 | - | 9 | 0.93 – 0.95 | 0.94 | Water Vapor |
| band09 | B10 | 9 | 10 | 1.36 – 1.38 | 1.37 | Cirrus |
| band10 | - | 10 | - | 10.60 – 11.19 | 10.895 | Thermal Infrared 1 |
| band11 | - | 11 | - | 11.50 – 12.51 | 12.005 | Thermal Infrared 2 |
The list of HLS v2.0 Data Known Issues is maintained at LP DAAC
☁️ Fmask omission (pre-2022 water/cloud-shadow)
❄️ Snow reflectance inconsistencies
📡 High-latitude multiple overpass fusions
🌫️ Bright surfaces: overestimated aerosol
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Land Surface Reflectance
HLS: Landsat 8/9 OLI
Reflectance (Nadir BRDF adjusted)
Repeat for HLS: Sentinal 2A/2B MSI
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We will examine S30 and L30 data from two dates and look for differences in EVI.
The Enhanced Vegetation Index (EVI) is a satellite-derived vegetation index designed to quantify plant “greenness” and improve on the widely used Normalized Difference Vegetation Index (NDVI). Like NDVI, it uses the contrast between red and near-infrared reflectance to measure vegetation density and health, but EVI also incorporates the blue band and additional correction factors. Specifically, EVI corrects for atmospheric scattering (e.g., from aerosols) and reduces the influence of soil background, which makes it more sensitive in areas of dense vegetation where NDVI tends to saturate. Because of this, EVI is especially useful for monitoring ecosystems with high biomass, detecting subtle changes in canopy structure, and improving accuracy in agricultural and forest studies.
The standard EVI formula is:
\[ EVI = G \times \frac{(NIR - RED)}{(NIR + C_1 \times RED - C_2 \times BLUE + L)} \]
\[ EVI_{L30} = 2.5 \times \frac{(band05 - band04)}{(band05 + 6 \times band04 - 7.5 \times band02 + 1)} \]
\[ EVI_{S30} = 2.5 \times \frac{(B8 - B4)}{(B8 + 6 \times B4 - 7.5 \times B2 + 1)} \]
| Component | Landsat 8/9 (HLS L30) | Wavelength Range (µm) | Sentinel-2 (HLS S30) | Wavelength Range (µm) |
|---|---|---|---|---|
| NIR | band05 | 0.85 – 0.88 | B08 | 0.784 – 0.899 |
| RED | band04 | 0.64 – 0.67 | B04 | 0.646 – 0.684 |
| BLUE | band02 | 0.45 – 0.51 | B02 | 0.458 – 0.523 |