ASTER geometric performance

doi:10.1109/TGRS.2005.849055

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ASTER geometric performance

2005-12-01

PRE

Akira Iwasaki *

DOI：10.1109/TGRS.2005.849055

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Abstract

En 中文

The Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) system acquires multispectral images ranging from the visible to thermal infrared region. The ASTER system consists of three subsystems: visible and near-infrared (VNIR), short-wave infrared (SWIR) and thermal infrared (TIR) radiometers. The VNIR subsystem has a backward-viewing telescope as well as a nadir one. To deliver data products of high quality from the viewpoint of geolocation and hand-to-hand registration performance, a fundamental program, called Level-1 data processing, has been developed for images obtained using four telescopes with a cross-track pointing function. In this work, the methodology of the geometric validation is first described. Next, the image quality of ASTER data products is evaluated in view of the geometric performance over a period of four years. The hand-to-hand registration accuracy in the subsystem is better than 0.1 pixels and that between subsystems is better than 0.2 pixels. This means that the geometric database is determined accurately and the image matching method based on a cross-correlation function is effective in the operational usage.

Keywords:

Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER)

geometric validation

image matching

image quality

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