Preflight Spectral Calibration of the Orbiting Carbon Observatory 2

This paper describes the preflight spectral calibration methods and results for the Orbiting Carbon Observatory 2 (OCO-2), following the approach developed for the first OCO. The instrument line shape (ILS) function and dispersion parameters were determined through laser-based spectroscopic measurem...

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Veröffentlicht in:IEEE transactions on geoscience and remote sensing 2017-05, Vol.55 (5), p.2499-2508
Hauptverfasser: Lee, Richard A. M., O'Dell, Christopher W., Wunch, Debra, Roehl, Coleen M., Osterman, Gregory B., Blavier, Jean-Francois, Rosenberg, Robert, Chapsky, Lars, Frankenberg, Christian, Hunyadi-Lay, Sarah L., Fisher, Brendan M., Rider, David M., Crisp, David, Pollock, Randy
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container_issue 5
container_start_page 2499
container_title IEEE transactions on geoscience and remote sensing
container_volume 55
creator Lee, Richard A. M.
O'Dell, Christopher W.
Wunch, Debra
Roehl, Coleen M.
Osterman, Gregory B.
Blavier, Jean-Francois
Rosenberg, Robert
Chapsky, Lars
Frankenberg, Christian
Hunyadi-Lay, Sarah L.
Fisher, Brendan M.
Rider, David M.
Crisp, David
Pollock, Randy
description This paper describes the preflight spectral calibration methods and results for the Orbiting Carbon Observatory 2 (OCO-2), following the approach developed for the first OCO. The instrument line shape (ILS) function and dispersion parameters were determined through laser-based spectroscopic measurements, and then further optimized by comparing solar spectra recorded simultaneously on the ground by the OCO-2 flight instrument and a collocated high-resolution Fourier transform spectrometer (FTS). The resulting ILS profiles and dispersion parameters, when applied to the FTS solar data, showed agreement between the spectra recorded by the spectrometers and FTS to approximately 0.2% RMS, satisfying the preflight spectral calibration accuracy requirement of
doi_str_mv 10.1109/TGRS.2016.2645614
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M. ; O'Dell, Christopher W. ; Wunch, Debra ; Roehl, Coleen M. ; Osterman, Gregory B. ; Blavier, Jean-Francois ; Rosenberg, Robert ; Chapsky, Lars ; Frankenberg, Christian ; Hunyadi-Lay, Sarah L. ; Fisher, Brendan M. ; Rider, David M. ; Crisp, David ; Pollock, Randy</creator><creatorcontrib>Lee, Richard A. M. ; O'Dell, Christopher W. ; Wunch, Debra ; Roehl, Coleen M. ; Osterman, Gregory B. ; Blavier, Jean-Francois ; Rosenberg, Robert ; Chapsky, Lars ; Frankenberg, Christian ; Hunyadi-Lay, Sarah L. ; Fisher, Brendan M. ; Rider, David M. ; Crisp, David ; Pollock, Randy</creatorcontrib><description>This paper describes the preflight spectral calibration methods and results for the Orbiting Carbon Observatory 2 (OCO-2), following the approach developed for the first OCO. The instrument line shape (ILS) function and dispersion parameters were determined through laser-based spectroscopic measurements, and then further optimized by comparing solar spectra recorded simultaneously on the ground by the OCO-2 flight instrument and a collocated high-resolution Fourier transform spectrometer (FTS). The resulting ILS profiles and dispersion parameters, when applied to the FTS solar data, showed agreement between the spectra recorded by the spectrometers and FTS to approximately 0.2% RMS, satisfying the preflight spectral calibration accuracy requirement of &lt;;0.25% RMS. 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M.</au><au>O'Dell, Christopher W.</au><au>Wunch, Debra</au><au>Roehl, Coleen M.</au><au>Osterman, Gregory B.</au><au>Blavier, Jean-Francois</au><au>Rosenberg, Robert</au><au>Chapsky, Lars</au><au>Frankenberg, Christian</au><au>Hunyadi-Lay, Sarah L.</au><au>Fisher, Brendan M.</au><au>Rider, David M.</au><au>Crisp, David</au><au>Pollock, Randy</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Preflight Spectral Calibration of the Orbiting Carbon Observatory 2</atitle><jtitle>IEEE transactions on geoscience and remote sensing</jtitle><stitle>TGRS</stitle><date>2017-05</date><risdate>2017</risdate><volume>55</volume><issue>5</issue><spage>2499</spage><epage>2508</epage><pages>2499-2508</pages><issn>0196-2892</issn><eissn>1558-0644</eissn><coden>IGRSD2</coden><abstract>This paper describes the preflight spectral calibration methods and results for the Orbiting Carbon Observatory 2 (OCO-2), following the approach developed for the first OCO. The instrument line shape (ILS) function and dispersion parameters were determined through laser-based spectroscopic measurements, and then further optimized by comparing solar spectra recorded simultaneously on the ground by the OCO-2 flight instrument and a collocated high-resolution Fourier transform spectrometer (FTS). The resulting ILS profiles and dispersion parameters, when applied to the FTS solar data, showed agreement between the spectra recorded by the spectrometers and FTS to approximately 0.2% RMS, satisfying the preflight spectral calibration accuracy requirement of &lt;;0.25% RMS. 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identifier ISSN: 0196-2892
ispartof IEEE transactions on geoscience and remote sensing, 2017-05, Vol.55 (5), p.2499-2508
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1558-0644
language eng
recordid cdi_proquest_journals_1879743988
source IEEE Electronic Library (IEL)
subjects Atmospheric measurements
Calibration
Carbon
Carbon dioxide (CO₂)
Detectors
Dispersion
dispersion parameters
Fourier transform spectrometers
Fourier transforms
instrument line shape (ILS)
Instruments
Laser applications
Lasers
Line shape
Measurement by laser beam
Observatories
Optimization
Orbiting Carbon Observatory 2 (OCO-2)
Parameters
Solar spectra
Spectra
spectral calibration
Spectrometers
Wavelength measurement
title Preflight Spectral Calibration of the Orbiting Carbon Observatory 2
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