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Sentinel 2 L1C & L2A

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Sentinel-2 is a European wide-swath, high-resolution (as defined by ESA) multispectral imaging mission. Its optical imagery supports applications such as land monitoring, emergency response, and security-related use cases. The multispectral instrument provides 13 spectral bands spanning the visible, near-infrared, and shortwave infrared regions.

Dedicated to supplying data for Copernicus services, Sentinel-2 carries a range of technologies such as multispectral imaging instruments for land, ocean, and atmospheric monitoring. It delivers high-resolution optical images for land monitoring, emergency response, and security services. For more information, see the S2 Mission and the Collection User Guide.

Basic Facts

PropertyValue
SensorMultiSpectral Instrument (MSI), 13 bands: 4 visible bands, 6 Near-Infrared bands, and 3 Short-Wave Infrared bands
Spatial resolution10 m, 20 m, and 60 m (band-dependent)
Revisit time5 days at the equator (2-3 days at mid latitudes)
Spatial coverageLand and coastal areas between latitudes 56°S and 83°N
Common use casesLand-cover mapping, land-change detection, vegetation monitoring, burned-area analysis

Product Differences

PropertySentinel-2 L1CSentinel-2 L2A
MeasurementTop-of-atmosphere (TOA) reflectanceBottom-of-atmosphere (BOA) reflectance, processed from L1C using Sen2Cor
Data availabilityAvailable since November 2015Available since October 2016 (global availability since January 2017)

Note: Sentinel-2A was maneuvered into a new orbit (located 36° away from Sentinel-2B) and resumed observations in 13 March 2025. With this campaign, the Sentinel-2 constellation consists of 3 satellites for 1 year (till 13 March 2026).[1]

Attribution and Use

EU law grants free access to Copernicus Sentinel Data and Service Information for the purpose of the following lawful uses: a) reproduction; b) distribution; c) communication to the public; d) adaptation, modification, and combination with other data and information; e) any combination of points a to d.

See more details on the use of Copernicus Sentinel data and service information.

Tracing based on Sentinel imagery is allowed for commercial purposes as well.

Acknowledgment: Contains modified Copernicus Sentinel data [Year] processed by Planet.

Accessing Sentinel-2 Data

To access data, you need to send a POST request to the Processing API. The requested data will be returned as the response to your request. Each POST request can be tailored to get exactly the data you require by setting various parameters depending on the data source.

Endpoint Locations

DataServiceNotes
Sentinel-2 L1Cservices.sentinel-hub.com/api/Global since November 2015
Sentinel-2 L2Aservices.sentinel-hub.com/api/Europe since November 2016
Global since January 2017

Data type identifiers:

  • sentinel-2-l1c
  • sentinel-2-l2a

Use these as the value of the input.data.type parameter in your API requests. This ensures you get the correct Sentinel-2 data level.

Filtering Options

This chapter explains the input.data.dataFilter object for Sentinel-2 data.

mosaickingOrder

Sets the order of overlapping tiles from which the output result is mosaicked. Tiles typically come from the same orbit/acquisition.

ValueDescriptionNotes
mostRecent(default) Pixel selected from the most recently acquired tileIn case multiple tiles share the same timestamp, the one downloaded or created latest will be used.
leastRecentSame as above, but in reverse order
leastCCPixel selected from tile with least cloud coverageTile-level metadata (each covering about 12,000 sq. km), approximate values

maxCloudCoverage

Sets the upper limit for cloud coverage (%) based on precomputed estimates in the tile metadata. For example, setting 20 retrieves only tiles with at most 20% cloud coverage.

note

The filter is per-tile and might not perfectly reflect the area of interest.

previewMode

Sentinel-2 L1C
Deprecated

As of April 15, 2025, new orbit and tile previews are no longer produced. All existing previews will be removed May 12, 2026.

The Sentinel Hub API supports both full- and low-resolution access. Low-resolution “previews” allow faster loading but have limitations.

ValueDescription
DETAIL (default)Full-resolution to 200 m/px – original files
TILE_PREVIEWUp to 640 m/px – tile previews (identical at 160 m/px)
PREVIEWUp to 1500 m/px – orbit-wide previews at 200 m/px
EXTENDED_PREVIEWAs PREVIEW but allows > 1500 m/px resolutions (up to 1 month old data)
note

maxCloudCoverage is ignored for PREVIEW and EXTENDED_PREVIEW.

Sentinel-2 L2A

Low-resolution previews are not generated for L2A. Full-resolution processing is available up to 1500 m per pixel, though performance degrades beyond 250 m/px.

ValueDescription
DETAILDisplays original data from full resolution to 1500 m per pixel

Processing Options

This chapter explains the input.data.processing object for Sentinel-2 data.

ParameterDescriptionValuesDefault
upsamplingInterpolation when requested resolution > source resolutionNEAREST - nearest neighbour interpolation
BILINEAR - bilinear interpolation
BICUBIC - bicubic interpolation
NEAREST
downsamplingInterpolation when requested resolution < source resolutionNEAREST - nearest neighbour interpolation
BILINEAR - bilinear interpolation
BICUBIC - bicubic interpolation
NEAREST

For visualization, see upsampling comparison examples.

Available Bands and Data

This chapter will explain the bands and data which can be set in the evalscript input object. Any string listed in the column Name can be an element of the input.bands array in your evalscript.

NameDescriptionResolutionNotes
B01Coastal aerosol60 m
B02Blue10 m
B03Green10 m
B04Red10 m
B05Vegetation red edge20 m
B06Vegetation red edge20 m
B07Vegetation red edge20 m
B08NIR10 m
B8ANarrow NIR20 m
B09Water vapour60 m
B10SWIR – Cirrus60 m(excluded for L2A BOA data)
B11SWIR20 m
B12SWIR20 m
CLPCloud probability (S2Cloudless) (more)160 mS2Cloudless band is 160 m; can be requested for products at any output resolution
CLMCloud mask (S2Cloudless) (more)160 m
AOT (L2A)Aerosol Optical Thickness map (Sen2Cor)10 mOnly L2A
SCL (L2A)Scene classification (Sen2Cor)20 mOnly L2A
SNW (L2A)Snow probability (Sen2Cor)20 mOnly L2A
CLD (L2A)Cloud probability (Sen2Cor)20 mOnly L2A
sunAzimuthAnglesSun azimuth angle5000 m
sunZenithAnglesSun zenith angle5000 m
viewAzimuthMeanViewing azimuth angle5000 m
viewZenithMeanViewing zenith angle5000 m
dataMaskMask of data/no data pixels (more)N/ACalculated per pixel

Units

The data values for each band in your evalscript are provided in the units specified below. You can set the desired unit via input.units in your evalscript setup function.

The available units and their meanings depend on the selected dataset and band. Refer to the dataset-specific sections below for details on value scaling and interpretation.

BandPhysical QuantitySentinel Hub UnitsSource FormatTypical Range
Optical bandsReflectance (unitless)REFLECTANCE (default)UINT150 – 0.4 *
Optical bandsDigital numbersDNUINT150 – 4000 *
CLPCloud probability (unitless) × 255DNUINT80 – 255
CLMCloud maskDNUINT80 (no clouds), 1 (clouds), 255 (no data)
L2A only: AOTAerosol optical thicknessOPTICAL_DEPTHUINT160 – 0.6 (AOT = DN / 1000)
L2A only: SCLScene classification maskDNUINT80 – No data; 1–11 classification codes
L2A only: SNWSnow probabilityPERCENTUINT80 – 100
L2A only: CLDCloud probabilityPERCENTUINT80 – 100
sunAzimuthAnglesAngle (degrees)DEGREESFLOAT3230 – 200
sunZenithAnglesAngle (degrees)DEGREESFLOAT3215 – 80
viewAzimuthMeanAngle (degrees)DEGREESFLOAT3290 – 300
viewZenithMeanAngle (degrees)DEGREESFLOAT320 – 12
dataMaskN/ADNN/A0 (no data), 1 (data)

*Higher values expected in IR bands; reflectance may exceed 1.

Harmonize Values

ESA updated the Sentinel-2 processing baseline starting with version 04.00 in January 2022, introducing changes to digital number (DN) interpretation that apply to this and all subsequent baselines.

For harmonized Sentinel-2 optical data, digital numbers (DN) are related to reflectance as:

  • DN = 10000 × reflectance

harmonizeValues can be true (default) or false, and it's behavior depends on the units chosen:

  • REFLECTANCE:
    • harmonizeValues = true: negative reflectance values are clamped to zero. In other words, pixels with negative reflectance return zero reflectance instead.
    • harmonizeValues = false: negative reflectance values can be returned.
  • DN:
    • harmonizeValues = true: DN values are harmonized so they are comparable with data from previous baselines. Therefore it still holds that DN = 10000 * REFLECTANCE. In addition, negative values are clamped to zero.
    • harmonizeValues = false: DN values are exactly as provided in the source files themselves. The "true" DN value, you could say. Don't forget that values have different definitions with different processing baselines, careful with mosaicking!

Mosaicking

All mosaicking types are supported.

Scenes Object

The scenes object stores metadata.

Example (L1C ORBIT mosaicking):

Property nameValue
dateFrom'2020-09-15T00:00:00Z'
dateTo'2020-09-15T00:00:00Z'
tiles[i].sentinel2ProductId'S2A_MSIL1C_20200915T101031_N0209_R022_T33TVM_20200915T122749'
tiles[i].date'2020-09-15T10:17:52Z'
tiles[i].shId11583048
tiles[i].cloudCoverage2.09
tiles[i].dataPath's3://sentinel-s2-l1c/tiles/33/T/VM/2020/9/15/0'

Collection Specific Constraints (Sentinel-2 L2A)

Atmospheric correction for Sentinel-2 L2A products is performed using ESA’s official Sen2Cor processor. This processing is carried out by ESA as part of the standard data production workflow.

Catalog API Capabilities

To access Sentinel-2 product metadata, send a search request to the Catalog API. The requested metadata is returned as a JSON response.

DatasetCollection IdentifierFilter ExtensionDistinct Extension
Sentinel-2 L1Csentinel-2-l1ceo:cloud_coverdate
Sentinel-2 L2Asentinel-2-l2aeo:cloud_coverdate