Mapping snow depth in open alpine terrain from stereo satellite imagery

To date, there is no definitive approach to map snow depth in mountainous areas from spaceborne sensors. Here, we examine the potential of very-high-resolution (VHR) optical stereo satellites to this purpose. Two triplets of 0.70 m resolution images were acquired by the Pléiades satellite over an op...

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Main Authors: R. Marti, S. Gascoin, E. Berthier, M. de Pinel, T. Houet, D. Laffly
Format: Article
Language:English
Published: Copernicus Publications 2016-07-01
Series:The Cryosphere
Online Access:http://www.the-cryosphere.net/10/1361/2016/tc-10-1361-2016.pdf
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author R. Marti
S. Gascoin
E. Berthier
M. de Pinel
T. Houet
D. Laffly
author_facet R. Marti
S. Gascoin
E. Berthier
M. de Pinel
T. Houet
D. Laffly
author_sort R. Marti
collection DOAJ
description To date, there is no definitive approach to map snow depth in mountainous areas from spaceborne sensors. Here, we examine the potential of very-high-resolution (VHR) optical stereo satellites to this purpose. Two triplets of 0.70 m resolution images were acquired by the Pléiades satellite over an open alpine catchment (14.5 km<sup>2</sup>) under snow-free and snow-covered conditions. The open-source software Ame's Stereo Pipeline (ASP) was used to match the stereo pairs without ground control points to generate raw photogrammetric clouds and to convert them into high-resolution digital elevation models (DEMs) at 1, 2, and 4 m resolutions. The DEM differences (dDEMs) were computed after 3-D coregistration, including a correction of a &minus;0.48 m vertical bias. The bias-corrected dDEM maps were compared to 451 snow-probe measurements. The results show a decimetric accuracy and precision in the Pléiades-derived snow depths. The median of the residuals is &minus;0.16 m, with a standard deviation (SD) of 0.58 m at a pixel size of 2 m. We compared the 2 m Pléiades dDEM to a 2 m dDEM that was based on a winged unmanned aircraft vehicle (UAV) photogrammetric survey that was performed on the same winter date over a portion of the catchment (3.1 km<sup>2</sup>). The UAV-derived snow depth map exhibits the same patterns as the Pléiades-derived snow map, with a median of &minus;0.11 m and a SD of 0.62 m when compared to the snow-probe measurements. The Pléiades images benefit from a very broad radiometric range (12 bits), allowing a high correlation success rate over the snow-covered areas. This study demonstrates the value of VHR stereo satellite imagery to map snow depth in remote mountainous areas even when no field data are available.
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spelling doaj.art-e9713ae8aa5b465890cdeea456929e332022-12-21T20:36:58ZengCopernicus PublicationsThe Cryosphere1994-04161994-04242016-07-011041361138010.5194/tc-10-1361-2016Mapping snow depth in open alpine terrain from stereo satellite imageryR. Marti0S. Gascoin1E. Berthier2M. de Pinel3T. Houet4D. Laffly5Géographie de l'Environnement (GEODE), UT2J/CNRS, Toulouse, FranceCentre d'Etudes Spatiales de la Biosphère (CESBIO), UPS/CNRS/IRD/CNES, Toulouse, FranceLaboratoire d'Etudes en Géophysique et Océanographie Spatiales, (LEGOS), UPS/CNRS/IRD/CNES, Toulouse, FranceGeoFalco, Longages, FranceGéographie de l'Environnement (GEODE), UT2J/CNRS, Toulouse, FranceGéographie de l'Environnement (GEODE), UT2J/CNRS, Toulouse, FranceTo date, there is no definitive approach to map snow depth in mountainous areas from spaceborne sensors. Here, we examine the potential of very-high-resolution (VHR) optical stereo satellites to this purpose. Two triplets of 0.70 m resolution images were acquired by the Pléiades satellite over an open alpine catchment (14.5 km<sup>2</sup>) under snow-free and snow-covered conditions. The open-source software Ame's Stereo Pipeline (ASP) was used to match the stereo pairs without ground control points to generate raw photogrammetric clouds and to convert them into high-resolution digital elevation models (DEMs) at 1, 2, and 4 m resolutions. The DEM differences (dDEMs) were computed after 3-D coregistration, including a correction of a &minus;0.48 m vertical bias. The bias-corrected dDEM maps were compared to 451 snow-probe measurements. The results show a decimetric accuracy and precision in the Pléiades-derived snow depths. The median of the residuals is &minus;0.16 m, with a standard deviation (SD) of 0.58 m at a pixel size of 2 m. We compared the 2 m Pléiades dDEM to a 2 m dDEM that was based on a winged unmanned aircraft vehicle (UAV) photogrammetric survey that was performed on the same winter date over a portion of the catchment (3.1 km<sup>2</sup>). The UAV-derived snow depth map exhibits the same patterns as the Pléiades-derived snow map, with a median of &minus;0.11 m and a SD of 0.62 m when compared to the snow-probe measurements. The Pléiades images benefit from a very broad radiometric range (12 bits), allowing a high correlation success rate over the snow-covered areas. This study demonstrates the value of VHR stereo satellite imagery to map snow depth in remote mountainous areas even when no field data are available.http://www.the-cryosphere.net/10/1361/2016/tc-10-1361-2016.pdf
spellingShingle R. Marti
S. Gascoin
E. Berthier
M. de Pinel
T. Houet
D. Laffly
Mapping snow depth in open alpine terrain from stereo satellite imagery
The Cryosphere
title Mapping snow depth in open alpine terrain from stereo satellite imagery
title_full Mapping snow depth in open alpine terrain from stereo satellite imagery
title_fullStr Mapping snow depth in open alpine terrain from stereo satellite imagery
title_full_unstemmed Mapping snow depth in open alpine terrain from stereo satellite imagery
title_short Mapping snow depth in open alpine terrain from stereo satellite imagery
title_sort mapping snow depth in open alpine terrain from stereo satellite imagery
url http://www.the-cryosphere.net/10/1361/2016/tc-10-1361-2016.pdf
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