Data Set ID:

Antarctic Peninsula 100 m Digital Elevation Model Derived from ASTER GDEM, Version 1

This data set provides a 100 meter resolution surface topography Digital Elevation Model (DEM) of the Antarctic Peninsula. The DEM is based on Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) Global Digital Elevation Model (GDEM) data.

NSIDC does not archive these data.

  • Coastal Processes > Coastal Elevation > COASTAL ELEVATION
  • Glaciers/Ice Sheets > Glacier Elevation/Ice Sheet Elevation > GLACIER ELEVATION/ICE SHEET ELEVATION
  • Topography > Terrain Elevation > TERRAIN ELEVATION
Data Format(s):
  • GeoTIFF
Spatial Coverage:
N: -63, 
S: -70, 
E: -55, 
W: -70
Spatial Resolution:
  • 100 m x 100 m
Temporal Coverage:
  • 1 January 2000 to 31 December 2009
Temporal ResolutionNot specifiedMetadata XML:View Metadata Record
Data Contributor(s):Allison Cook

Geographic Coverage

Please contact the data provider for the correct Data Citation for this data set.

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Detailed Data Description

This data set provides a high-resolution Digital Elevation Model (DEM) of the Antarctic Peninsula.

dem map
Figure 1. 100-meter Digital Elevation Model of the Antarctic Peninsula 
High Resolution Image


The DEM is provided in GeoTIFF format and as an ASCII text file.

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File and Directory Structure

Table 1 contains the descriptions of the files in the data set.

Table 1. File Description
File Name Description


Final GeoTIFF file.


Ancillary GeoTIFF files

  • aux: Auxilliary text file
  • rrd: Pyramid file
  • xml: XML file


DEM in ASCII text format.

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File Naming Convention

Files are named according to the following convention and as described in Table 2.

File name example: APDEM100m.tif



Table 2. File Naming Convention
Variable Description


Antarctic Peninsula


Digital Elevation Model


Resolution (100 meter)


File extension

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File Size

Data files range in size from 1 KB to 209 MB.

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The entire data set is approximately 600 MB.

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Spatial Coverage

Antarctic Peninsula
Northernmost Latitude: 70°S
Southernmost Latitude: 63°S
Westernmost Longitude: 70° W
Easternmost Longitude: 55° W

Spatial Resolution

100 m

Projection and Grid Description

Projection: WGS84 Antarctic Polar Sterographic, Standard Parallel -71 deg South.

Grid: Surface elevation model, 1 Band, Continuous, Floating point, 32 Bit, 6164 columns, 8918 rows.

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Temporal Coverage

This DEM is based on the ASTER GDEMv1, which uses scenes dating from 2000 to 2009. The dates of all scenes used to generate the GDEM in this region are not specified.

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Parameter or Variable

Elevation in meters above the EGM96 Geoid. The EGM96 Geoid is a DEM consisting of elevations above the WGS84 Ellipsoid.

Parameter Range

0 to 3172 meters

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Software and Tools

Data are readable using standard image processing software.

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Data Acquisition and Processing

Data Acquisition Methods

Data used to created this DEM were modified from the ASTER Global Digital Elevation Model (GDEM).The ASTER GDEM is the most recently released nearly global elevation data set and is based upon a composition of automatically generated DEMs from ASTER stereo scenes acquired from 2000 to the present. It was produced by the Ministry of Economy, Trade and Industry (METI) of Japan and the United States National Aeronautics and Space Administration (NASA). Full details of the methodology for this data set are to be published in Cook, et. al., 2012.

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Derivation Techniques and Algorithms

No formal ASTER GDEM validation has been performed over Antarctica, but it is evident that there are significant errors within the tiles throughout the Antarctic Peninsula region, introduced as a direct result of high reflectance and lack of features on snow-covered plateaus. Since conventional data correction techniques do not work in this region, a new approach was used to significantly improve the data set. Processing for the new DEM converted the GDEM into contours and removed the erroneous contours, producing a smooth and realistic new DEM from the remaining contours. This method was applied only to poor-quality regions of the GDEM, and the resulting DEMs were merged with the unaltered high-quality GDEM regions. See Figure 2 for the edited regions. The method is made possible by the fact that the high-artefact regions are those where the real-surface (as observed on the Landsat Image Mosaic of Antarctica [LIMA]) is smooth and has a low slope angle.

map of edited regions
Figure 2. This map shows regions that were edited from the raw GDEM.

Processing Steps

ASTER GDEM tiles were downloaded from ASTER GDEM site and mosaicked according to each latitudinal degree across the Antarctic Peninsula. Each mosaic was projected onto a reference system suitable for minimizing distortions in scale and for preserving angles locally. In this case, Lambert Conformal Conic (LCC) projection was used with standard parallels and other parameters according to latitude. The subsequent methodology was then applied separately to each latitudinal degree raster between 63 degrees and 70 degrees South.

Using a Geographic Information System (GIS), contours were generated automatically from the GDEM at 20 m intervals. A new file was then created by digitizing around regions of erroneous contours, based on the GDEM stacking number file and manual corrections using visible band imagery. These "noisy" regions of the DEM were then resampled to 200 m to simplify and remove gross errors, and sinks in the DEM were filled and smoothed. Contours at 20 m intervals were then created for this generalized DEM.

In order to correct these contours a slope model was created and contours that fell within a slope angle of greater than 20 degrees were removed. Secondly, contours less than 1 km in length were deleted, as these came from spikes or pits in the DEM. The surface topography was reconstructed by interpolation between the remaining contours, which represented consistent elevation values between the anomalies. The corrected regions of the DEM were then mosaicked with the remaining high-quality regions to create a topographically consistent DEM. The final step of the process involved reprojecting all tiles to a common reference system (Polar Stereographic projection with a standard latitude of 71 degrees South and a central meridian of 0 degrees), mosaicking all tiles and clipping to remove any remaining artifacts along the coast. The outer limit is based on the LIMA coastline with a 500 m buffer.

Error Sources

The new DEM has a mean elevation difference of - 4 m (±25 m Root Mean Square Error [RMSE]) from ICESat, and a horizontal error of less than 2 pixels, although elevation accuracies are lower on mountain peaks and steep-sided slopes. Some anomalies along the coast have been removed, resulting in small gaps, and the DEM has a small number of remaining artifacts. It only covers regions included in ASTER GDEM, in which there are inherent gaps and some missing islands.

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Sensor or Instrument Description

Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) nadir and backward looking sensors. The data set was based on the ASTER Global Digital Elevation Model (GDEM) data.

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References and Related Publications

Contacts and Acknowledgments

Alison Cook, Tavi Murray, and Adrian Luckman
Department of Geography
Swansea University
Swansea, SA2 8PP
United Kingdom

David G. Vaughan and Nicholas E. Barrand
British Antarctic Survey
High Cross, Madingley Road
Cambridge, CB3 0ET
United Kingdom

Document Information


April 18, 2012

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