Abstract

Quantitative geomorphic research depends on accurate topographic data often collected via remote sensing. Lidar, and photogrammetric methods like structure-from-motion, provide the highest quality data for generating digital elevation models (DEMs). Unfortunately, these data are restricted to relatively small areas, and may be expensive or time-consuming to collect. Global and near-global DEMs with 1 arcsec (∼30 m) ground sampling from spaceborne radar and optical sensors offer an alternative gridded, continuous surface at the cost of resolution and accuracy. Accuracy is typically defined with respect to external datasets, often, but not always, in the form of point or profile measurements from sources like differential Global Navigation Satellite System (GNSS), spaceborne lidar (e.g., ICESat), and other geodetic measurements. Vertical point or profile accuracy metrics can miss the pixel-to-pixel variability (sometimes called DEM noise) that is unrelated to true topographic signal, but rather sensor-, orbital-, and/or processing-related artifacts. This is most concerning in selecting a DEM for geomorphic analysis, as this variability can affect derivatives of elevation (e.g., slope and curvature) and impact flow routing. We use (near) global DEMs at 1 arcsec resolution (SRTM, ASTER, ALOS, TanDEM-X, and the recently released Copernicus) and develop new internal accuracy metrics to assess inter-pixel variability without reference data. Our study area is in the arid, steep Central Andes, and is nearly vegetation-free, creating ideal conditions for remote sensing of the bare-earth surface. We use a novel hillshade-filtering approach to detrend long-wavelength topographic signals and accentuate short-wavelength variability. Fourier transformations of the spatial signal to the frequency domain allows us to quantify: 1) artifacts in the un-projected 1 arcsec DEMs at wavelengths greater than the Nyquist (twice the nominal resolution, so > 2 arcsec); and 2) the relative variance of adjacent pixels in DEMs resampled to 30-m resolution (UTM projected). We translate results into their impact on hillslope and channel slope calculations, and we highlight the quality of the five DEMs. We find that the Copernicus DEM, which is based on a carefully edited commercial version of the TanDEM-X, provides the highest quality landscape representation, and should become the preferred DEM for topographic analysis in areas without sufficient coverage of higher-quality local DEMs.

Highlights

  • Digital elevation models (DEMs) with accurate representations of topographic variability are vital to modern quantitative geomorphology

  • We focus only on slope as it is the first derivative of elevation, and inaccuracies caused by low inter-pixel consistency in this metric will manifest in other DEM derivatives, such as curvature and aspect

  • We choose to present the results of the geomorphic analysis in the discussion section, as they are pertinent to discussions of inter-pixel consistency, and to the suggestions and caveats of DEM selection

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Summary

Introduction

Digital elevation models (DEMs) with accurate representations of topographic variability are vital to modern quantitative geomorphology. With the recent release of the Copernicus global DEM (Fahrland et al, 2020; Leister-Taylor et al, 2020) at 30 m resolution (10 m in Europe), the community is faced with an additional choice besides the 30 m Advanced Spaceborne Thermal Emission and Reflection Radiometer Global DEM v3 (ASTER-GDEMv3; Abrams et al, 2020; Abrams and Crippen, 2019), reprocessed Shuttle Radar Topography Mission NASADEM (SRTM-NASADEM; Farr et al, 2007; Crippen et al, 2016; Buckley et al, 2020), and Advanced Land Observing Satellite World 3D v3.1 (ALOS-W3Dv3.1; Tadono et al, 2014; Takaku et al, 2014; EORC, 2021). Additional edited DEMs have been derived from these sources with the specific intention of hydrologic correction and flow routing (e.g., MERIT and MERIT Hydro; Yamazaki et al, 2017)

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