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The Orbiting Carbon Observatory (OCO) mission

  • Author(s): Crisp, D
  • Atlas, RM
  • Breon, FM
  • Brown, LR
  • Burrows, JP
  • Ciais, P
  • Connor, BJ
  • Doney, SC
  • Fung, IY
  • Jacob, DJ
  • Miller, CE
  • O'Brien, D
  • Pawson, S
  • Randerson, JT
  • Rayner, P
  • Salawitch, RJ
  • Sander, SP
  • Sen, B
  • Stephens, GL
  • Tans, PP
  • Toon, GC
  • Wennberg, PO
  • Wofsy, SC
  • Yung, YL
  • Kuang, Z
  • Chudasama, B
  • Sprague, G
  • Weiss, B
  • Pollock, R
  • Kenyon, D
  • Schroll, S
  • et al.
Abstract

The Orbiting Carbon Observatory (OCO) mission will make the first global, space-based measurements of atmospheric carbon dioxide (CO 2 ) with the precision, resolution, and coverage needed to characterize CO 2 sources and sinks on regional scales. The measurement approach and instrument specifications were determined through an analysis of existing carbon cycle data and a series of observing system simulation experiments. During its 2-year mission, OCO will fly in a 1:15 PM sun-synchronous orbit with a 16-day ground-track repeat time, just ahead of the EOS Aqua platform. It will carry a single instrument that incorporates three bore-sighted high-resolution spectrometers designed to measure reflected sunlight in the 0.76-μm O 2 A-band and in the CO 2 bands at 1.61 and 2.06 μm. Soundings recorded in these three bands will be used to retrieve the column-averaged CO 2 dry air mole fraction (X CO2 ). A comprehensive validation program was included in the mission to ensure that the space-based X CO2 measurements have precisions of ∼0.3% (1 ppm) on regional scales. OCO measurements will be used in global synthesis inversion and data assimilation models to quantify CO 2 sources and sinks. While OCO will have a nominal lifetime of only 2 years, it will serve as a pathfinder for future long-term CO 2 monitoring missions. © 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.

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