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Scientific and Technical Aerospace Reports Volume 38 July 28, 2000

Scientific and Technical Aerospace Reports Volume 38 July 28, 2000

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<strong>2000</strong>0064542 NASA Ames Research Center, Moffett Field, CA USA<br />

Issues in Absolute Spectral Radiometric Calibration: Intercomparison of Eight Sources<br />

Goetz, Alex<strong>and</strong>er F. H., Colorado Univ., USA; Kindel, Bruce, Colorado Univ., USA; Pilewskie, Peter, NASA Ames Research<br />

Center, USA; Summaries of the Seventh JPL Airborne Earth Science Workshop January 12-16, 1998; Dec. 19, 1998; <strong>Volume</strong> 1,<br />

pp. 169-174; In English; See also <strong>2000</strong>0064520<br />

Contract(s)/Grant(s): 95-B26; NAG5-4447; No Copyright; Avail: CASI; A02, Hardcopy; A04, Microfiche<br />

The application of atmospheric models to AVIRIS <strong>and</strong> other spectral imaging data to derive surface reflectance requires that<br />

the sensor output be calibrated to absolute radiance. Uncertainties in absolute calibration are to be expected, <strong>and</strong> claims of 92%<br />

accuracy have been published. Measurements of accurate surface albedos <strong>and</strong> cloud absorption to be used in radiative balance<br />

calculations depend critically on knowing the absolute spectral-radiometric response of the sensor. The Earth Observing System<br />

project is implementing a rigorous program of absolute radiometric calibration for all optical sensors. Since a number of imaging<br />

instruments that provide output in terms of absolute radiance are calibrated at different sites, it is important to determine the errors<br />

that can be expected among calibration sites. Another question exists about the errors in the absolute knowledge of the exoatmospheric<br />

spectral solar irradiance.<br />

Derived from text<br />

Calibrating; Optical Measuring Instruments; Radiance; Atmospheric Models; Radiometers<br />

<strong>2000</strong>0064543 Jet Propulsion Lab., California Inst. of Tech., Pasadena, CA USA<br />

Apparent Surface Reflectance of the DOE ARM SGP CART Central Site Derived from AVIRIS Spectral Images<br />

Green, Robert O., Jet Propulsion Lab., California Inst. of Tech., USA; Summaries of the Seventh JPL Airborne Earth Science<br />

Workshop January 12-16, 1998; Dec. 19, 1998; <strong>Volume</strong> 1, pp. 175-184; In English; See also <strong>2000</strong>0064520; No Copyright; Avail:<br />

CASI; A02, Hardcopy; A04, Microfiche<br />

The primary objective of the Department of Energy (DOE) Atmospheric Radiation Measurement (ARM) Program at the<br />

Southern Great Plains (SGP) Cloud <strong>and</strong> Radiation Testbed (CART) is to acquire in situ <strong>and</strong> remote sensing data to improve cloud<br />

<strong>and</strong> atmospheric radiative models <strong>and</strong> parameterizations. As a consequence of this program, a large number of atmosphere <strong>and</strong><br />

surface measurements are being acquired at the ARM SGP CART central site. NASA’s Airborne Visible/Infrared Imaging<br />

Spectrometer (AVIRIS) overflew this site on August 1, 1997. AVIRIS measures the upwelling spectral solar radiance from 400<br />

to 2500 nm at 10-nm intervals. From 20 km altitude, these calibrated spectra are acquired as images of 11 by up to 800 km with<br />

20-by-20 m spatial resolution. These data were acquired at the ARM SGP CART Central Site to first investigate derivation of<br />

atmospheric parameters from the measured spectra, second study the variation of these parameters, <strong>and</strong> third demonstrate the<br />

inversion of the calibrated radiance spectra to apparent surface reflectance. These objectives have been pursued with AVIRIS data<br />

at other sites for atmospheric water vapor <strong>and</strong> derivation of apparent surface reflectance.<br />

Derived from text<br />

Parameterization; Remote Sensing; Spectral Reflectance; Surface Properties; Radiance<br />

<strong>2000</strong>0064544 Jet Propulsion Lab., California Inst. of Tech., Pasadena, CA USA<br />

Minimum High Fire Temperatures Detected in AVIRIS Spectral Measurements from Brazil in 1995<br />

Green, Robert O., Jet Propulsion Lab., California Inst. of Tech., USA; Summaries of the Seventh JPL Airborne Earth Science<br />

Workshop January 12-16, 1998; Dec. 19, 1998; <strong>Volume</strong> 1, pp. 185-192A; In English; See also <strong>2000</strong>0064520; No Copyright; Avail:<br />

CASI; A02, Hardcopy; A04, Microfiche<br />

In August <strong>and</strong> September of 1995 the Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) was deployed to Brazil as<br />

part of the NASA Smoke Cloud Aerosol <strong>and</strong> Radiation experiment in Brazil (SCAR-B). AVIRIS measures spectra from 400 to<br />

2500 nm at 10-nm intervals. These spectra are acquired as images with dimensions of 11 by up to 800 km with 20-m spatial resolution.<br />

Spectral images measured by AVIRIS are spectrally, radiometrically, <strong>and</strong> spatially calibrated. During the SCAR-B deployment,<br />

AVIRIS measured more than 300 million spectra of regions of Brazil. A portion of these spectra were acquired over areas<br />

of actively burning fires. Actively burning fires emit radiance in the AVIRIS spectral range as a function of temperature. This<br />

emitted radiance is expressed from the 2500-nm end of the AVIRIS spectrum to shorter wavelengths as a function of intensity<br />

<strong>and</strong> modeled by the Planck function.. The objective of this research <strong>and</strong> analysis was to use spectroscopic methods to determine<br />

the minimum high temperature of the most intense fires measured in the SCAR-B AVIRIS data set. Spectra measured by AVIRIS<br />

with hot sources have been previously examined for volcanic lava <strong>and</strong> fires in Brazil.<br />

Derived from text<br />

Forest Fires; Imaging Spectrometers; Infrared Imagery; Radiance; Spectrum Analysis; Remote Sensing; High Temperature<br />

108

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