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An Overview of Solar Reflectance Remote Sensing Methods for Earth Science Applications. S. Platnick Laboratory for Atmospheres NASA Goddard Space Flight Center, Greenbelt MD USA. SORCE Science Team Meeting Sonoma CA 5 December 2003. Outline
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An Overview of Solar Reflectance Remote Sensing Methods for Earth Science Applications S. Platnick Laboratory for Atmospheres NASA Goddard Space Flight Center, Greenbelt MD USA SORCE Science Team Meeting Sonoma CA 5 December 2003
Outline • Solar reflectance remote sensing - a brief overview of passive solar techniques (excluding UV) • space-borne/aircraft techniques and instruments • examples w/emphasis on atmosphere (clouds and aerosols) • Radiometric calibration • radiance vs. irradiance • Solar spectral irradiance issues • use/misuse of irradiance data sets • 3.7 µm spectral band
Solar Reflectance Satellite Measurement Summary (incomplete) Key: Instrument development/management (other than US) Satellite platform S. Platnick, SORCE, 5 Dec 2003
H2O = --O3-- O2 O2 O2 VIS NIR SWIR MWIR SWIR CO2 CH4 N2O CO2 MODTRAN, absorption transmittance only Spectral regions of interest S. Platnick, SORCE, 5 Dec 2003
– general purpose window bands (land, aerosol, clouds) – ocean color/phytoplankton/ biogeo. chemistry – water vapor bands cloud particle size fire detection MODTRAN, absorption transmittance only MODIS (Terra, Aqua) nominal band locations S. Platnick, SORCE, 5 Dec 2003
MODTRAN, absorption transmittance only AVHRR nominal bands locations (channel 1, 2, 3) S. Platnick, SORCE, 5 Dec 2003
MODIS Land Surface Albedo, band 2 (0.86 µm)global animation for 2001, 16 day averages(derived from operational product MOD43, E. Moody, et al.) Click Here to See Movie S. Platnick, SORCE, 5 Dec 2003
MODIS land classification map (MOD12) urban MODIS 0.86 µm albedo, mid-late July 2001 S. Platnick, SORCE, 5 Dec 2003
1.0 Fine Aerosol Fraction 0.0 0.0 0.25 0.5 Aerosol Optical Thickness MODIS Aerosol Product -daily examples from 2001(MOD04, L3 1° gridded, Kaufman, Tanre, Remer, et al.) Click to See Movie S. Platnick, SORCE, 5 Dec 2003
MODIS Cloud Product – thermodynamic phase(MOD06, L3 0.1° gridded, Terra, 21 Nov 2003; modis-atmos.gsfc.nasa.gov) Uncertain Ice Liquid S. Platnick, SORCE, 5 Dec 2003
MODIS Cloud Product – optical thickness(MOD06, L3 0.1° gridded, Terra, 21 Nov 2003; modis-atmos.gsfc.nasa.gov) S. Platnick, SORCE, 5 Dec 2003
MODIS Cloud Product – particle effective radius(MOD06, L3 0.1° gridded, Terra, 21 Nov 2003; modis-atmos.gsfc.nasa.gov) S. Platnick, SORCE, 5 Dec 2003
MODTRAN, absorption transmittance only MISR (Terra) nominal bands locations 9 cameras ± 70 deg views S. Platnick, SORCE, 5 Dec 2003
MISR 9-camera animation over southern Florida(true-color composite) Click to See Movie S. Platnick, SORCE, 5 Dec 2003
MODTRAN, absorption transmittance only polarization channels POLDER (CNES, ADEOS-I,II) CCD array, rotating filter wheel S. Platnick, SORCE, 5 Dec 2003
1520 UTC 1539 Cloud Observations with AirPOLDER(19 minutes of data, Proteus Aircraft, CRYSTAL-FACE, 3 July 2002) S. Platnick, SORCE, 5 Dec 2003
Cloud Observations with AirPOLDER(19 minutes of data, Proteus Aircraft, CRYSTAL-FACE, 3 July 2002) Click to See Movie Click to See Movie RGB: 865(pol), 865(total), 763(total) Total radiance RGB: 865, 763, 443 nm (figs. courtesy of Jerome Riedi, U. Lille, France) S. Platnick, SORCE, 5 Dec 2003
* * * useful for stability as well as absolute cal Calibration for reflectance-based remote sensing • Fundamental measurement isbidirectional reflectance not radiance, • defined for some spectral band as: • where, • = viewing zenith angle, 0 = solar zenith angle • I() = spectral radiance (intensity) measured in viewing direction • F0, = solar spectral irradiance • Calibration approaches: • 1. Radiance calibration + solar spectral irradiance table —> reflectance • 2. On-board reflectance calibration (e.g., MODIS, MERIS, etc.) • 3. Other: vicarious calibration (ground-based validation), lunar observations, inter-satellite comparisons, etc. S. Platnick, SORCE, 5 Dec 2003
1. Radiance-based approach Reflectance uncertainty is: • Il difficulties compared with F0,l : • Lack of spaceborne absolute radiometery for imagers (e.g, absolute detectors, electrical substitution radiometers) • low energy(narrowband), short pixel dwell time (especially scanners, ~300 µs for MODIS 1km bands) • even if possible (microbolometer), would have to measure solid angle FOV in addition to aperture area • Difficulty in transferring standards, e.g., standard irradiance lamp transferred to radiance via diffuse plate to integrating sphere • Fortunately, remote sensing needs typically much less stringent than energy budget measurements (though stability still critical!) S. Platnick, SORCE, 5 Dec 2003
EOS SWIXR UA SWIR EOS VXR UA VNIR GSFC LXR Integrating Sphere calibration intercomparison(relative to SBRS SIS100 sphere cal) 100 (LXR/LSIS - 1) 100 (LXR/LSIS - 1) wavelength (nm) wavelength (nm) water vapor bands Butler et al., J. Res. NIST, 108, May-June 2003. (figs. courtesy of Jim Butler, NASA GSFC) S. Platnick, SORCE, 5 Dec 2003
MODTRAN Landsat ETM+ ASTER personal use MODIS (backup to refl. cal.) 1. Radiance-based approach, cont. Reflectance uncertainty is: • F0,l from published compilations and/or measurements: • 1974 NASA spectrum (Thekaekara, 1974 ): UV/VIS [CV-990 flights, Thekaekara (1969), JPL a/c program, Drummond (1967-68)], NIR-MWIR [3 published papers] • 1981 WRC spectrum: 0.3-1.25 µm [Neckel and Labs (1981) Jungfraujoch, spectral improvement, absolute pinned to WRC solar constant], Other spectral regions [Smith and Gottlieb (1974), Heath and Thekaekara (1977), Arvesen et al. (1969)] • 1984, Neckel and Labs: 0.33-1.25 µm (improved spectral w/Kitt Peak FTS, not absolute) • 1995, Kurucz: UV-SWIR compilation using Jungfraujoch, Kitt Peak, JPL/ATMOS, …; adopted by MODTRAN • 1998, 2002, Thuillier et al.: UV-SWIR, ATLAS SOLSPEC, SOSP EURECA • 20??: SORCE SIM S. Platnick, SORCE, 5 Dec 2003
MODIS band-averaged reflectance differencerelative to MODTRAN solar irradiance spectrum (Kurucz) S. Platnick, SORCE, 5 Dec 2003
1. Radiance-based approach, cont. • NOTE: A very uncomfortable uncertainty in the 3.7 µm band solar irradiance! Data sources include (?): • Thekaekara et al. (1974) – at 100 nm spectral resolution • Kondratyev, Andreev, Badinov, Grishechkin, and Popova (1965) – at 3.0, 3.6, 4.0 µm • ? Farmer and Norton (1989), Farmer et al. (1994), Livingston and Wallace (1991) • Example comparison between KABGP & Thekaekara et al. at 3.6 µm shows irradiance difference of about 15%, e.g., • Thekaekara et al. = 1.4 mW-cm-2-µm-1 • KABGP = 1.2 mW-cm-2-µm-1 S. Platnick, SORCE, 5 Dec 2003
MODIS Terra granulecoastal Chile/Peru (18 July 2001, 1530 UTC) phase retrieval RGB true-color composite uncertain ice liquid water no retrieval S. Platnick, SORCE, 5 Dec 2003
40 -1.0 32 24 -1.5 16 8 0 -2.0 3.7 µm retrieved re (Thekaekara) Dre (KABGP - Thekaekara) ice clouds MODIS Terra granule, coastal Chile/Peru (18 July 2001, 1530 UTC) S. Platnick, SORCE, 5 Dec 2003
calibration schematic Sun 1.4 % screen optional 7.8 % screen (bands 8-16 saturate w/o screen) MODIS Spectralon diffuser panel 58.1 SDSM to scan mirror SD 20.5 20.7 MODIS Solar Diffuser Stability Monitor instrument (integrating sphere, 9 filters, 0.4-1 µm; views sun w/screen & panel) 2. Reflectance-based approach(MODIS example, VIS-SWIR) S. Platnick, SORCE, 5 Dec 2003
Difference relative to NIST (%) viewing angle (deg) Laboratory Laboratory panel BRDF measurements (relative to NIST)Spectralon at l=633 nm Early et al., J. Atmos. Oceanic Tech., 17, August 2000. (figs. courtesy of Jim Butler, NASA GSFC) S. Platnick, SORCE, 5 Dec 2003
MODIS Solar Diffuser Degradation (fig. courtesy of Bill Barnes, Jack Xiong, NASA GSFC) S. Platnick, SORCE, 5 Dec 2003
Satellite Instruments w/Solar Diffusers (incomplete?) • Used for primary calibration • – MODIS, MERIS (?) • Used for trending • – MISR, SeaWiFS (primary methods are vicarious calibration) • Not used • – ETM+ (due to apparent diffuser degradation relative to vicarious calibration and pre-flight cal) S. Platnick, SORCE, 5 Dec 2003
Solar Remote Sensing Summary • Fundamental measurement needed for geophysical retrievals typically reflectance (not radiance) • Absolute calibration not as stringent as irradiance energy budget requirements, but stability critical for climate monitoring • New generation of satellite sensors w/on-board solar reflectance panels, flown with varying degrees of success • Accurate solar spectral irradiance needed across the solar spectrum • – Radiance-based calibration methods —> reflectance • – Intercomparison of reflectance and radiance-based methods • – Traceability of reflectance-based radiometry to MKS standards • 3.7 µm band for cloud re retrievals: heritage(AVHRR) and new (MODIS, CERES group) studies subject to unknown solar irradiance uncertainty S. Platnick, SORCE, 5 Dec 2003
Solar satellite-borne techniques missing from the table: • Temporal (Geosynchronous imagers) • Solar occultation (transmittance) measurements for stratospheric trace gases • NASA New Millenium technology demonstrations (EO-1) • ??? S. Platnick, SORCE, 5 Dec 2003
MODTRAN, absorption transmittance only Landsat TM nominal bands locations (1, 2, 3, 4, 5, 7) S. Platnick, SORCE, 5 Dec 2003
MODTRAN, absorption transmittance only dual views ASTER (Terra) NASDA/JAXA S. Platnick, SORCE, 5 Dec 2003
MODTRAN, absorption transmittance only MOPITT (Terra) 2.2-2.4 µm bands, nominal locations (gas correlation radiometry) CH4 CO S. Platnick, SORCE, 5 Dec 2003
1.0 Fine Aerosol Fraction 0.0 0.0 0.25 0.5 Aerosol Optical Thickness MODIS Aerosol Product - global animation, 2001(MOD04, L3 1° gridded, Kaufman, Tanre, Remer, et al.) Click to See Movie S. Platnick, SORCE, 5 Dec 2003
Land surface polarization(RGB: 2250, 865, 410 nm color composite, RSP a/c instrument) Reflectance Polarized Reflectance (figs. courtesy of Brian Cairns, NASA GISS/U. Columbia) S. Platnick, SORCE, 5 Dec 2003
Cloud Observations with POLDER Stratocumulus over the ocean Scattering Angle Namibia Color composite 443-670-865 nm Same scene in polarized light • Polarization features less affected by multiple scattering than total radiance (figs. courtesy of Bréon, François-Marie, LSCE, France) S. Platnick, SORCE, 5 Dec 2003
MODIS calibration schematic Sun SDSM Views: Sun, SD, Dark 1.44% Screen Optional 7.8% Screen (Bands 8-16 saturate w/o screen) SDSM 58.1 To Scan Mirror SD 20.5 20.7
MODIS Instrument Degradation/Drift S. Platnick, SORCE, 5 Dec 2003
MODIS Instrument Degradation/Drift (fig. courtesy of Bill Barnes, Jack Xiong, NASA GSFC) S. Platnick, SORCE, 5 Dec 2003