The on-orbit performance of the Orbiting Carbon Observatory-2 (OCO-2) instrument and its radiometrically calibrated products
By David Crisp. 2016
420 citations recorded by the source corpus.
Abstract. The Orbiting Carbon Observatory-2 (OCO-2) carries and points a three-channel imaging grating spectrometer designed to collect high-resolution, co-boresighted spectra of reflected sunlight within the molecular oxygen (O2) A-band at 0.765 microns and the carbon dioxide (CO2) bands at 1.61 and 2.06 microns. These measurements are calibrated and then combined into soundings that are analyzed to retrieve spatially resolved estimates of the column-averaged CO2 dry-air mole fraction, XCO2. Variations of XCO2 in space and time are then analyzed in the context of the atmospheric transport to quantify surface sources and sinks of CO2. This is a particularly challenging remote-sensing observation because all but the largest emission sources and natural absorbers produce only small ( To meet its demanding measurement requirements, each OCO-2 spectrometer channel collects 24 spectra s−1 across a narrow ( 17 000), dynamic range (∼ 104), and sensitivity (continuum signal-to-noise ratio > 400). The OCO-2 instrument performance was extensively characterized and calibrated prior to launch. In general, the instrument has performed as expected during its first 18 months in orbit. However, ongoing calibration and science analysis activities have revealed a number of subtle radiometric and spectroscopic challenges that affect the yield and quality of the OCO-2 data products. These issues include increased numbers of bad pixels, transient artifacts introduced by cosmic rays, radiance discontinuities for spatially non-uniform scenes, a misunderstanding of the instrument polarization orientation, and time-dependent changes in the throughput of the oxygen A-band channel. Here, we describe the OCO-2 instrument, its data products, and its on-orbit performance. We then summarize calibration challenges encountered during its first 18 months in orbit and the methods used to mitigate their impact on the calibrated radiance spectra distributed to the science community.
Subfields: Atmospheric Science, Global and Planetary Change, Spectroscopy
View Paper: https://www.semanticscholar.org/paper/87200856e95a91f1ddd69e0c9ba100aff7293442
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In Atmospheric Science
- Paul O. Wennberg
- David Crisp
- Christopher W. O'Dell
- Brendan M. Fisher
- Annmarie Eldering
- Matthäus Kiel
- Paul I. Palmer
- Liang Feng
In Global and Planetary Change
- Paul I. Palmer
- Liang Feng
- Paul O. Wennberg
- David Crisp
- Christopher W. O'Dell
- Brendan M. Fisher
- Annmarie Eldering
- Matthäus Kiel
In Spectroscopy
Citations in the corpus
- How bias correction goes wrong: measurement of XCO2 affected by erroneous surface pressure estimates (2019, background): “(2014) Bialystok, Poland Deutscher et al. (2014) Manaus, Brazil Dubey et al. (2014) Burgos, Phillipines Velazco et al. (2017) Ny Ålesund, Spitzbergen, Norway Notholt et al.”
- Improved retrievals of carbon dioxide from Orbiting Carbon Observatory-2 with the version 8 ACOS algorithm (2018, methodology): “The latter is related to a slope in the observed radiance within an individual sounding’s field-of-view, and is determined from OCO-2’s color slices as discussed in Crisp et al. (2017).”