DEA Surface Reflectance OA (Landsat 5 TM)

DEA Surface Reflectance OA (Landsat 5 TM)

Geoscience Australia Landsat 5 TM Observation Attributes Collection 3

Version:

3.0.0 (Latest)

Product types:

Baseline, Raster

Time span:

16 Aug 1986 – 17 Nov 2011

Update frequency:

Daily

Product ID:

ga_ls5t_ard_3

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About

DEA Surface Reflectance OA (Landsat 5 TM) is part of a suite of Digital Earth Australia (DEA)’s Surface Reflectance datasets that represent the vast archive of images captured by the US Geological Survey (USGS) Landsat and European Space Agency (ESA) Sentinel-2 satellite programs, validated, calibrated, and adjusted for Australian conditions — ready for easy analysis.

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Code examples

Code sample

Key details

Collection

Geoscience Australia Landsat Collection 3

Persistent ID

130853

Licence

Creative Commons Attribution 4.0 International Licence

Cite this product

Data citation

Fuqin, Li., Jupp, D.L.B., Sixsmith, J., Wang, L., Dorj, P., Vincent, A., Alam, I., Hooke, J., Oliver, S., Thankappan, M., 2019. GA Landsat 5 TM Analysis Ready Data Collection 3. Geoscience Australia, Canberra. https://pid.geoscience.gov.au/dataset/ga/130853

Background

Sub-product

This is a sub-product of DEA Surface Reflectance (Landsat 5 TM). See the parent product for more information.

The contextual information related to a dataset is just as valuable as the data itself. This information, also known as data provenance or data lineage, includes details such as the data’s origins, derivations, methodology and processes. It allows the data to be replicated and increases the reliability of derivative applications.

Data that is well-labelled and rich in spectral, spatial and temporal attribution can allow users to investigate patterns through space and time. Users are able to gain a deeper understanding of the data environment, which could potentially pave the way for future forecasting and early warning systems.

The surface reflectance data produced by NBAR and NBART requires accurate and reliable data provenance. Attribution labels, such as the location of cloud and cloud shadow pixels, can be used to mask out these particular features from the surface reflectance analysis, or used as training data for machine learning algorithms. Additionally, the capacity to automatically exclude or include pre-identified pixels could assist with emerging multi-temporal and machine learning analysis techniques.

What this product offers

This product contains a range of pixel-level observation attributes (OA) derived from satellite observation, providing rich data provenance:

  • null pixels

  • clear pixels

  • cloud pixels

  • cloud shadow pixels

  • snow pixels

  • water pixels

  • spectrally contiguous pixels

  • terrain shaded pixels

It also features the following pixel-level information pertaining to satellite, solar and sensing geometries:

  • solar zenith

  • solar azimuth

  • satellite view

  • incident angle

  • exiting angle

  • azimuthal incident

  • azimuthal exiting

  • relative azimuth

  • timedelta

Technical information

How observation attributes can be used

This product provides pixel- and acquisition-level information that can be used in a variety of services and applications. This information includes:

  • data provenance, which:

    • denotes which inputs/parameters were used in running the algorithm

    • demonstrates how a particular result was achieved

    • can be used as evidence for the reasoning behind particular decisions

    • enables traceability

  • training data for input into machine learning algorithms, or additional likelihood metrics for image feature content, where pre-classified content includes:

    • cloud

    • cloud shadow

    • snow

    • water

  • additional pixel filtering (e.g. exclude pixels with high incident angles)

  • pre-analysis filtering based on image content (e.g. return acquisitions that have less than 10% cloud coverage)

  • input into temporal statistical summaries to produce probability estimates on classification likelihood

This product allows you to screen your data for undesired anomalies that can occur during any phase: from the satellite’s acquisition, to the processing of surface reflectance, which relies on various auxiliary sources each having their own anomalies and limitations.

Pixel-level information on satellite and solar geometries is useful if you wish to exclude pixels that might be deemed questionable based on their angular measure. This is especially useful if you are using the NBAR product, where pixels located on sloping surfaces can exhibit a lower than expected surface reflectance due to a higher incidence or solar zenith angle.

Example - Terrain shadow and high incident angles

These images depict an area containing high topographic relief, terrain shadow, and high incident angles. Applications, such as water classification, can mis-classify dark regions as water due to the effect of high incident angles in regions of high topographic relief.

NBAR, terrain shadow, high incident angle, NBAR+ mask overlay, NBART

Figure 1. (A) Surface Reflectance (Landsat 5 TM NBAR) image; (B) terrain shadow mask; (C) high incident angle mask (>65); (D) NBAR+ mask overlay; (E) equivalent Surface Reflectance (Landsat 5 TM NBART) image.

Terminology for satellite, solar and sensing geometries

  • Zenith The point in the sky or celestial sphere directly above a point of interest (in this case, the point being imaged on Earth).

  • Solar zenith (degrees) The angle between the zenith and the centre of the sun’s disc.

  • Solar azimuth (degrees) The angle of the sun’s position from true north; i.e. the angle between true north and a vertical circle passing through the sun and the point being imaged on Earth.

  • Satellite view or satellite zenith (degrees) The angle between the zenith and the satellite.

  • Satellite azimuth (degrees) The angle of the satellite’s position from true north; i.e. the angle between true north and a vertical circle passing through the satellite and the point being imaged on Earth.

  • Incident angle (degrees) The angle between a ray incident on a surface and the line perpendicular to the surface at the point of incidence.

  • Exiting angle (degrees) The angle between a ray reflected from a surface and the line perpendicular to the surface at the point of emergence.

  • Azimuthal incident (degrees) The angle between true north and the incident direction in the slope geometry.

  • Azimuthal exiting (degrees) The angle between true north and the exiting direction in the slope geometry.

  • Relative azimuth (degrees) The relative azimuth angle between the sun and view directions.

  • Relative slope (degrees) The relative azimuth angle between the incident and exiting directions in the slope geometry.

  • Timedelta (seconds) The time from satellite apogee (the point of orbit at which the satellite is furthest from the Earth).

Zenith angles

Figure 2. Zenith angles. Image modified from Support to Aviation Control Service (2011).

Zenith and azimuth angles

Figure 3. Zenith and azimuth angles. θs = solar zenith; θν = satellite view; Φs = solar azimuth (green); Φν = satellite azimuth (blue); Φ = relative azimuth (red). Image modified from Hudson et al. (2006).

Incident (i) and exiting (e) angles

Figure 4. Incident (i) and exiting (e) angles for a level and inclined surface. Image modified from Dymond and Shepherd (1999).

The Fmask algorithm

Fmask allows you to have pre-classified image content for use within their applications. This can include:

  • additional confidence metrics in image content classifiers

  • pre-labelled data for machine learning classifiers

  • pixel screening for cloud and cloud shadow

  • on-the-fly mapping applications for water and snow

The result of the Fmask algorithm contains mutually exclusive classified pixels, and the numerical schema for the pixels are as follows:

  • 0 = null

  • 1 = clear

  • 2 = cloud

  • 3 = cloud shadow

  • 4 = snow

  • 5 = water

The spectrally contiguous pixels which have a valid observation in each spectral band. This is particularly useful for applications undertaking band math, as it allows non-contiguous data to be ignored during the band math evaluation or masked during post-evaluation. The product can be utilised as a strict mask, and the numerical schema for the pixels are as follows:

  • 0 = non-contiguous

  • 1 = contiguous

The terrain-shaded pixels product can be utilised as a strict mask and exclude pixels that were unobservable by the sun or sensor. The numerical schema for the pixels are as follows:

  • 0 = shaded

  • 1 = not shaded

Different types of terrain-shaded pixels

Figure 5. Different types of terrain-shaded pixels. C = point of interest; D = point located along the direction of the sun; 90-θS = solar zenith; Z0 = elevation at location C; Zd = elevation at location D. Image sourced from Jupp et al. (2012).

Example - Fmask

Some analyses might want to exclude targets that are obscured by cloud or cloud shadow. This is particularly useful for applications looking to harvest statistical information for particular regions of interest, such as field crops, where large swaths of data aren’t required to be loaded into computer memory. Instead, only the regions of interest are loaded, analysed and summarised, reducing computational costs.

The following images represent the surface reflectance image and derived Fmask classification result for visual context. The colours for the Fmask classification are displayed as:

  • Black = clear

  • Magenta = cloud

  • Yellow = cloud shadow

  • Cyan = snow

  • Dark blue = water

False colour composite and the resulting Fmask classification

Figure 6. (A) False colour composite; (B) the resulting Fmask classification.

For this product, the Fmask dataset has had the object dilation for the cloud and cloud shadow layers removed. This enables you to customise object dilation to meet your needs for specific applications. For example, one application might work better having a 7-pixel dilation, whereas another might require 5.

You can also choose your own kernel shape and size in which to apply a particular dilation. Dilation can be useful for filling holes within objects and extending the edges of detected objects. It is important to note that small objects (e.g. 1 or 2 pixels in size) will be dilated and become large objects. If this is an undesired outcome, it is best to filter out any small objects prior to applying dilation filters.

For more information on dilation, see:

Other uses of Fmask:

  • For training data for use with machine learning classifiers Fmask can help refine the result and produce a more accurate classification result. The data can also be combined with other classifiers, creating a confidence metric that users can then filter by. For example, you can filter cloud pixels rated >70% as a combined metric from the combination of cloud classifiers.

  • For input into a statistical summary It can provide another information product that can be used to indicate the probability of being a particular classified feature. For example, a statistical summary of cloud and/or cloud shadow can highlight pixels that are consistently being detected as a cloud or cloud shadow. As clouds and cloud shadows are non-persistent features, pixels with a high cloud or cloud shadow frequency can be labelled or attributed as highly probable of not being cloud or cloud shadow.

Image format specifications

Fmask

Format

GeoTIFF

Resolution

30m

Datatype

UInt8

Classification ENUM

0 = null
1 = clear
2 = cloud
3 = cloud shadow
4 = snow
5 = water

Valid data range

[0,5]

Tiled with X and Y block sizes

512x512

Compression

Deflate, Level 9, Predictor 2

Pyramids

Levels: [8,16,32]
Compression: deflate
Resampling: mode
Overview X&Y block sizes: 512x512

Contrast stretch

None

Output CRS

As specified by source dataset; source is UTM with WGS84 as the datum

nbar-contiguity, nbart-contiguity

Format

GeoTIFF

Resolution

30m

Datatype

UInt8

Classification ENUM

0 = non-contiguous (spectral information not present in each band)
1 = contiguous (spectral information present in each band)

Valid data range

[0,1]

Tiled with X and Y block sizes

512x512

Compression

Deflate, Level 9, Predictor 2

Pyramids

Levels: [8,16,32]
Compression: deflate
Resampling: GDAL default (nearest)
Overview X&Y block sizes: 512x512

Contrast stretch

None

Output CRS

As specified by source dataset; source is UTM with WGS84 as the datum

combined-terrain-shadow

Format

GeoTIFF

Resolution

30m

Datatype

UInt8

Classification ENUM

0 = terrain shadow
1 = not terrain shadow

Valid data range

[0,1]

Tiled with X and Y block sizes

512x512

Compression

Deflate, Level 9, Predictor 2

Pyramids

None

Contrast stretch

None

Output CRS

As specified by source dataset; source is UTM with WGS84 as the datum

incident, exiting, azimuthal-incident, azimuthal-exiting, relative-azimuth, relative-slope, timedelta

Format

GeoTIFF

Resolution

30m

No data value

NaN (IEEE 754)

Tiled with X and Y block sizes

512x512

Compression

Deflate, Level 9, Predictor 2

Pyramids

None

Contrast stretch

None

Output CRS

As specified by source dataset; source is UTM with WGS84 as the datum

Processing steps

  1. Longitude and Latitude Calculation

  2. Satellite and Solar Geometry Calculation

  3. Elevation Retrieval and Smoothing

  4. Slope and Aspect Calculation

  5. Incidence and Azimuthal Incident Angles Calculation

  6. Exiting and Azimuthal Exiting Angles Calculation

  7. Relative Slope Calculation

  8. Terrain Occlusion Mask

  9. Function of Mask (Fmask)

  10. Contiguous Spectral Data Mask Calculation

Accuracy

For information on the accuracy of the algorithms for test locations, see Zhu and Woodcock (2012) and Zhu, Wang and Woodcock (2015).

Limitations

Fmask

Fmask has limitations due to the complex nature of detecting natural phenomena, such as cloud. For example, bright targets, such as beaches, buildings and salt lakes often get mistaken for clouds.

Fmask is designed to be used as an immediate/rapid source of information screening. The idea is that over a temporal period enough observations will be made to form a temporal likelihood. For example, if a feature is consistently being masked as cloud, it is highly probable that it is not cloud. As such, derivative processes can be created to form an information layer containing feature probabilities.

Edges and fringes of clouds tend to be more opaque and can be missed by the cloud detection algorithm. In this instance, applying a morphological dilation will grow the original cloud object and capture edges and fringes of clouds. However, it is important to note that other cloud objects could also be dilated. Be mindful of single-pixel objects that could grow to become large objects. Consider filtering out these small objects prior to analysis.

Angular measurement and shadow classification

The Digital Elevation Model (DEM) is used for identifying terrain shadow, as well as producing incident and exiting angles. It is derived from the Shuttle Radar Topography Mission (SRTM) and produced with approximately 30 m resolution. As such, any angular measurements and shadow classifications are limited to the precision of the DEM itself. The DEM is known to be noisy across various locations, so to reduce any potential extrema, a Gaussian smooth is applied prior to analysis.

Quality assurance

The authors evaluated the Fmask algorithm using a total of 188 randomly selected Worldwide Reference System (WRS) locations across nine latitudinal zones. From these locations, 212 Landsat scenes were used as a reference set as part of the accuracy assessment. The average accuracy for cloud detection was 96.4%.

The calculation of the satellite and solar positional geometry datasets are largely influenced by the publicly available ephemeris data and whether the satellite has an on-board GPS, as well as the geographical information that resides with the imagery data and the metadata published by the data providers. The code to generate the geometry grids is routinely tested and evaluated for accuracy at >6 decimal places of precision.

The technical report containing the data summary for the Phase 1 DEA Surface Reflectance Validation is available: DEA Analysis Ready Data Phase 1 Validation Project : Data Summary

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How to access the data

Open Data Cube

This product is contained in the Open Data Cube instance managed by Digital Earth Australia (DEA). This simplified process allows you to query data from its sub-products as part of a single query submitted to the database.

See Analysis Ready Data: example queries

Old versions

View previous versions of this data product.

2.0.0: DEA Pixel Quality (Landsat)

2.0.0: DEA Pixel Quality Count (Landsat)

Acknowledgments

This research was undertaken with the assistance of resources from the National Computational Infrastructure (NCI), which is supported by the Australian Government.

Landsat level 0 and level 1 data courtesy of the U.S. Geological Survey.

The authors would like to thank the following organisations:

  • National Aeronautics and Space Administration (NASA)

  • Environment Canada

  • The Commonwealth Scientific and Industrial Research Organisation (CSIRO)

  • National Oceanic and Atmospheric Administration (NOAA) / Earth System Research Laboratories (ESRL) / Physical Sciences Laboratory (PSD)

  • The National Geospatial-Intelligence Agency (NGA)

  • The United States Geological Survey (USGS) / Earth Resources Observation and Science (EROS) Center

  • Spectral Sciences Inc.