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HLS Burn Scars
This is a repackaging, not a new dataset. It is HLS Burn Scars by IBM-NASA Geospatial (Phillips, Roy, Ankur, Ramachandran), NASA / USGS HLS, converted to TACO. Pixel values and labels are kept as released except where the description below says otherwise. All credit belongs to the original authors: if you use it, please cite them and follow their licence.
original dataset · paper · licence: CC-BY-4.0
Repackaged into TACO by the Image and Signal Processing Group (ISP), Universitat de València, within the ELLIOT project.
Citation
Please cite the original work:
@software{HLS_Foundation_2023,
author = {Phillips, Christopher and Roy, Sujit and Ankur, Kumar and Ramachandran, Rahul},
title = {{HLS Foundation Burnscars Dataset}},
month = aug,
year = {2023},
doi = {10.57967/hf/0956},
url = {https://huggingface.co/ibm-nasa-geospatial/hls_burn_scars}
}
About the data
804 Harmonized Landsat Sentinel-2 (HLS S30) scenes of 512x512 px at 30 m over burn scars in the contiguous United States: six bands of surface reflectance with a binary burned-area mask. Converted from the original GeoTIFFs.
804 samples · splits: train 540 · validation 264 · tasks: semantic-segmentation
Packaged as TACO v3.
Full description
Splits. The official directory split, 540 train and 264 val. The release has no test split, and its own split is not MGRS-tile disjoint: 124 of 365 tiles appear on both sides, at different dates.
Radiometry. Reflectance is kept as float32 in physical units.
Nodata. The masks' -1 marks unlabelled pixels, and is rewritten as 255 and declared as the ignore index; the GeoTIFF headers claim nodata=-1000, which occurs nowhere in the data. The imagery's declared nodata of 0.0 is not propagated, because 0.0 is a real reflectance minimum in the blue band and honouring it would mask valid dark pixels.
Getting started
git clone --recursive https://github.com/OscarPellicer/taco
pip install -e "taco/python[ml]" # builds the reader: C++23, CMake, Ninja, pkg-config, libcurl >= 7.83, OpenSSL >= 3
Read it straight from the Hub:
import os
from huggingface_hub import hf_hub_download, snapshot_download
from taco.ml import Dataset, plot_sample
path = hf_hub_download("isp-uv-es/hls-burn-scars-taco", "hls-burn-scars.zip", repo_type="dataset")
ds = Dataset(path)
plot_sample(ds[0])
or from a local copy:
ds = Dataset("hls-burn-scars.zip")
sample = ds[0] # {slot name: SlotValue}, arrays decoded
sample["hls"].array.shape
Metadata without decoding anything:
import taco
taco.read("hls-burn-scars.zip") # one Arrow table, levels joined
Samples
What a sample contains
| role | slot | holds | modality | detail |
|---|---|---|---|---|
| input | hls |
raster | multispectral | 6 band(s), unit 1, physical |
| target | burned |
mask | label_raster | 2 classes |
Licence
CC-BY-4.0
Providers: IBM-NASA Geospatial (Phillips, Roy, Ankur, Ramachandran), NASA / USGS HLS
Acknowledgements
TACO was designed by César Aybar and is specified at https://asterisk.coop/taco/spec/.
Built by Oscar Pellicer within the ELLIOT project at the Image and Signal Processing Group (ISP), Universitat de València.
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