Preflight Radiometric Calibration of Orbiting Carbon Observatory 2
The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitor...
Ausführliche Beschreibung
Autor*in: |
Rosenberg, Robert [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
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2017 |
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Übergeordnetes Werk: |
Enthalten in: IEEE transactions on geoscience and remote sensing - New York, NY : IEEE, 1964, 55(2017), 4, Seite 1994-2006 |
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Übergeordnetes Werk: |
volume:55 ; year:2017 ; number:4 ; pages:1994-2006 |
Links: |
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DOI / URN: |
10.1109/TGRS.2016.2634023 |
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Katalog-ID: |
OLC1992307113 |
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520 | |a The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. | ||
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650 | 4 | |a Calibration | |
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700 | 1 | |a Maxwell, Stephen |4 oth | |
700 | 1 | |a Johnson, B. Carol |4 oth | |
700 | 1 | |a Chapsky, Lars |4 oth | |
700 | 1 | |a Lee, Richard A. M |4 oth | |
700 | 1 | |a Pollock, Randy |4 oth | |
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10.1109/TGRS.2016.2634023 doi PQ20170501 (DE-627)OLC1992307113 (DE-599)GBVOLC1992307113 (PRQ)c1592-194a7267e7bc3ba645bcd9fabc1d93a49a1bba04665ec4d65e9830b74a8e54640 (KEY)0048677920170000055000401994preflightradiometriccalibrationoforbitingcarbonobs DE-627 ger DE-627 rakwb eng 620 550 DNB Rosenberg, Robert verfasserin aut Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. Integrating sphere NIST Orbiting Carbon Observatory (OCO-2) Extraterrestrial measurements Carbon Radiometry Observatories Instruments Calibration remote sensing Measurement Research Radiation Analysis Maxwell, Stephen oth Johnson, B. Carol oth Chapsky, Lars oth Lee, Richard A. M oth Pollock, Randy oth Enthalten in IEEE transactions on geoscience and remote sensing New York, NY : IEEE, 1964 55(2017), 4, Seite 1994-2006 (DE-627)129601667 (DE-600)241439-9 (DE-576)015095282 0196-2892 nnns volume:55 year:2017 number:4 pages:1994-2006 http://dx.doi.org/10.1109/TGRS.2016.2634023 Volltext http://ieeexplore.ieee.org/document/7809060 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-ARC SSG-OLC-TEC SSG-OLC-GEO SSG-OLC-FOR SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_70 AR 55 2017 4 1994-2006 |
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10.1109/TGRS.2016.2634023 doi PQ20170501 (DE-627)OLC1992307113 (DE-599)GBVOLC1992307113 (PRQ)c1592-194a7267e7bc3ba645bcd9fabc1d93a49a1bba04665ec4d65e9830b74a8e54640 (KEY)0048677920170000055000401994preflightradiometriccalibrationoforbitingcarbonobs DE-627 ger DE-627 rakwb eng 620 550 DNB Rosenberg, Robert verfasserin aut Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. Integrating sphere NIST Orbiting Carbon Observatory (OCO-2) Extraterrestrial measurements Carbon Radiometry Observatories Instruments Calibration remote sensing Measurement Research Radiation Analysis Maxwell, Stephen oth Johnson, B. Carol oth Chapsky, Lars oth Lee, Richard A. M oth Pollock, Randy oth Enthalten in IEEE transactions on geoscience and remote sensing New York, NY : IEEE, 1964 55(2017), 4, Seite 1994-2006 (DE-627)129601667 (DE-600)241439-9 (DE-576)015095282 0196-2892 nnns volume:55 year:2017 number:4 pages:1994-2006 http://dx.doi.org/10.1109/TGRS.2016.2634023 Volltext http://ieeexplore.ieee.org/document/7809060 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-ARC SSG-OLC-TEC SSG-OLC-GEO SSG-OLC-FOR SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_70 AR 55 2017 4 1994-2006 |
allfields_unstemmed |
10.1109/TGRS.2016.2634023 doi PQ20170501 (DE-627)OLC1992307113 (DE-599)GBVOLC1992307113 (PRQ)c1592-194a7267e7bc3ba645bcd9fabc1d93a49a1bba04665ec4d65e9830b74a8e54640 (KEY)0048677920170000055000401994preflightradiometriccalibrationoforbitingcarbonobs DE-627 ger DE-627 rakwb eng 620 550 DNB Rosenberg, Robert verfasserin aut Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. Integrating sphere NIST Orbiting Carbon Observatory (OCO-2) Extraterrestrial measurements Carbon Radiometry Observatories Instruments Calibration remote sensing Measurement Research Radiation Analysis Maxwell, Stephen oth Johnson, B. Carol oth Chapsky, Lars oth Lee, Richard A. M oth Pollock, Randy oth Enthalten in IEEE transactions on geoscience and remote sensing New York, NY : IEEE, 1964 55(2017), 4, Seite 1994-2006 (DE-627)129601667 (DE-600)241439-9 (DE-576)015095282 0196-2892 nnns volume:55 year:2017 number:4 pages:1994-2006 http://dx.doi.org/10.1109/TGRS.2016.2634023 Volltext http://ieeexplore.ieee.org/document/7809060 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-ARC SSG-OLC-TEC SSG-OLC-GEO SSG-OLC-FOR SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_70 AR 55 2017 4 1994-2006 |
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10.1109/TGRS.2016.2634023 doi PQ20170501 (DE-627)OLC1992307113 (DE-599)GBVOLC1992307113 (PRQ)c1592-194a7267e7bc3ba645bcd9fabc1d93a49a1bba04665ec4d65e9830b74a8e54640 (KEY)0048677920170000055000401994preflightradiometriccalibrationoforbitingcarbonobs DE-627 ger DE-627 rakwb eng 620 550 DNB Rosenberg, Robert verfasserin aut Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. Integrating sphere NIST Orbiting Carbon Observatory (OCO-2) Extraterrestrial measurements Carbon Radiometry Observatories Instruments Calibration remote sensing Measurement Research Radiation Analysis Maxwell, Stephen oth Johnson, B. Carol oth Chapsky, Lars oth Lee, Richard A. M oth Pollock, Randy oth Enthalten in IEEE transactions on geoscience and remote sensing New York, NY : IEEE, 1964 55(2017), 4, Seite 1994-2006 (DE-627)129601667 (DE-600)241439-9 (DE-576)015095282 0196-2892 nnns volume:55 year:2017 number:4 pages:1994-2006 http://dx.doi.org/10.1109/TGRS.2016.2634023 Volltext http://ieeexplore.ieee.org/document/7809060 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-ARC SSG-OLC-TEC SSG-OLC-GEO SSG-OLC-FOR SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_70 AR 55 2017 4 1994-2006 |
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10.1109/TGRS.2016.2634023 doi PQ20170501 (DE-627)OLC1992307113 (DE-599)GBVOLC1992307113 (PRQ)c1592-194a7267e7bc3ba645bcd9fabc1d93a49a1bba04665ec4d65e9830b74a8e54640 (KEY)0048677920170000055000401994preflightradiometriccalibrationoforbitingcarbonobs DE-627 ger DE-627 rakwb eng 620 550 DNB Rosenberg, Robert verfasserin aut Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 2017 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. Integrating sphere NIST Orbiting Carbon Observatory (OCO-2) Extraterrestrial measurements Carbon Radiometry Observatories Instruments Calibration remote sensing Measurement Research Radiation Analysis Maxwell, Stephen oth Johnson, B. Carol oth Chapsky, Lars oth Lee, Richard A. M oth Pollock, Randy oth Enthalten in IEEE transactions on geoscience and remote sensing New York, NY : IEEE, 1964 55(2017), 4, Seite 1994-2006 (DE-627)129601667 (DE-600)241439-9 (DE-576)015095282 0196-2892 nnns volume:55 year:2017 number:4 pages:1994-2006 http://dx.doi.org/10.1109/TGRS.2016.2634023 Volltext http://ieeexplore.ieee.org/document/7809060 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-ARC SSG-OLC-TEC SSG-OLC-GEO SSG-OLC-FOR SSG-OPC-GGO SSG-OPC-GEO GBV_ILN_70 AR 55 2017 4 1994-2006 |
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620 550 DNB Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 Integrating sphere NIST Orbiting Carbon Observatory (OCO-2) Extraterrestrial measurements Carbon Radiometry Observatories Instruments Calibration remote sensing Measurement Research Radiation Analysis |
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IEEE transactions on geoscience and remote sensing |
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Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 |
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title_full |
Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 |
author_sort |
Rosenberg, Robert |
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IEEE transactions on geoscience and remote sensing |
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IEEE transactions on geoscience and remote sensing |
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10.1109/TGRS.2016.2634023 |
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preflight radiometric calibration of orbiting carbon observatory 2 |
title_auth |
Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 |
abstract |
The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. |
abstractGer |
The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. |
abstract_unstemmed |
The imaging spectrometers of the second orbiting carbon observatory were radiometrically calibrated before launch during instrumentlevel ground testing. The gain and dark responses were characterized for each focal plane array detector element. An integrating sphere source with an integrated monitoring spectroradiometer illuminated the OCO-2 spectrometers at many light levels. Instrument output was compared with the calibrated output of the source to derive gain coefficients. This source was calibrated in situ with respect to the National Institute of Standards and Technology reference standards, and the instrument met its absolute performance requirement of 5%. Matching fields of view for the internal monitor detectors and the external instrument under test was found to be particularly important, as observed in the results and supported by modeling. Temperature-dependent dark offsets were corrected in a separate process. Solar spectra with varying neutral density filters were used to validate the linearity of the spectrometers. |
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4 |
title_short |
Preflight Radiometric Calibration of Orbiting Carbon Observatory 2 |
url |
http://dx.doi.org/10.1109/TGRS.2016.2634023 http://ieeexplore.ieee.org/document/7809060 |
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false |
author2 |
Maxwell, Stephen Johnson, B. Carol Chapsky, Lars Lee, Richard A. M Pollock, Randy |
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