The ASTER Digital Elevation Model (AST14DEM) product is generated using bands 3N (nadir-viewing) and 3B (backward-viewing) of an ASTER Level 1A image acquired by the Visible and Near Infrared (VNIR) sensor. The VNIR subsystem includes two independent telescope assemblies that facilitate the generation of stereoscopic data. The band 3 stereo pair is acquired in the spectral range of 0.78 and 0.86 microns with a base-to-height ratio of 0.6 and an intersection angle of 27.7 degrees. There is a time lag of approximately one minute between the acquisition of the nadir and backward images.For a better understanding, refer to this diagram depicting the along-track imaging geometry of the ASTER VNIR nadir and backward-viewing sensors.
The accuracy of the new LP DAAC produced DEMs will meet or exceed accuracy specifications set for the ASTER relative DEMs by the Algorithm Theoretical Basis Document (ATBD). Users likely will find that the DEMs produced by the new LP DAAC system have accuracies approaching those specified in the ATBD for absolute DEMs. Validation testing has shown that DEMs produced by the new system frequently are more accurate than 25 meters root mean square error (RMSE) in xyz dimensions.
Starting in early summer of 2006, LP DAAC has implemented new production software for efficiently creating quality DEMs. Based on an automated stereo-correlation method, the new software generates a relative DEM without any ground control points (GCPs). It utilizes the ephemeris and attitude data derived from both the ASTER instrument and the Terra spacecraft platform. The new ASTER DEM is a single band product with 30 meter horizontal postings that is geodetically referenced to the UTM coordinate system and to the Earth's geoid using the EGM96 geopotential model. Compared to ASTER DEMs previously available from the LP DAAC, users likely will note some differences in ASTER DEMs produced by the new system. These differences are due to the DEMs no being produced automatically with no manual editing. Larger water bodies are detected and typically have a single value, but they no longer are manually edited. Any failed areas, while infrequent, remain as they occur. Cloudy areas typically appear as bright regions, rather than as manually edited dark areas.
|File Size||~12 MB|
|Temporal Extent||2000-03-06 to Present|
|Coordinate System||Universal Transverse Mercator (UTM)|
|Datum||World Geodetic System (WGS84)|
|Geographic Dimensions||~60 km x 60 km|
|Number of Science Dataset (SDS) Layers||1|
|Columns/Rows||Varies by scene x Varies by scene|
|Pixel Size||30 m|
|SDS Name||Description||Units||Data Type||Fill Value||No Data Value||Valid Range||Scale Factor|
|Band 1||Digital Elevation Model||Meters||16-bit signed integer||N/A||N/A||-32768 to 32768||N/A|