<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>K. Aral</dc:contributor>
  <dc:contributor>S. Hook</dc:contributor>
  <dc:contributor>H. Kieffer</dc:contributor>
  <dc:contributor>H. Lang</dc:contributor>
  <dc:contributor>T. Matsunaga</dc:contributor>
  <dc:contributor>A. Ono</dc:contributor>
  <dc:contributor>F. D. Palluconi</dc:contributor>
  <dc:contributor>H. Sakuma</dc:contributor>
  <dc:contributor>P. Slater</dc:contributor>
  <dc:contributor>T. Takashima</dc:contributor>
  <dc:contributor>H. Tonooka</dc:contributor>
  <dc:contributor>S. Tsuchida</dc:contributor>
  <dc:contributor>R.M. Welch</dc:contributor>
  <dc:contributor>E. Zalewski</dc:contributor>
  <dc:creator>K. Thome</dc:creator>
  <dc:date>1998</dc:date>
  <dc:description>&lt;p&gt;&lt;span&gt;Describes the preflight and inflight calibration approaches used for the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER). The system is a multispectral, high-spatial resolution sensor on the Earth Observing System's EOS-AM1 platform. Preflight calibration of ASTER uses well-characterized sources to provide calibration and preflight round-robin exercises to understand biases between the calibration sources of ASTER and other EOS sensors. These round-robins rely on well-characterized, ultra-stable radiometers. An experiment field in Yokohama, Japan, showed that the output from the source used for the visible and near-infrared (VNIR) subsystem of ASTER may be underestimated by 1.5%, but this is still within the 4% specification for the absolute, radiometric calibration of these bands. Inflight calibration will rely on vicarious techniques and onboard blackbodies and lamps. Vicarious techniques include ground-reference methods using desert and water sites. A recent joint field campaign gives confidence that these methods currently provide absolute calibration to better than 5%, and indications are that uncertainties less than the required 4% should be achievable at launch. The EOS-AM1 platform will also provide a spacecraft maneuver that will allow ASTER to see the Moon, allowing further characterization of the sensor. A method for combining the results of these independent calibration results is presented. The paper also describes the plans for validating the Level 2 data products from ASTER. These plans rely heavily upon field campaigns using methods similar to those used for the ground-reference, vicarious calibration methods.&lt;/span&gt;&lt;/p&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1109/36.701023</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>IEEE</dc:publisher>
  <dc:title>ASTER preflight and inflight calibration and the validation of level 2 products</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>