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OCO-3 (Orbiting Carbon Observatory 3)

NASA carbon-monitoring instrument deployed on ISS in May 2019; SIF at 757 nm and 740 nm demonstrated; target-mode and snapshot area mode provide hundreds to thousands of SIF retrievals per overpass at biologically diverse sites.

OCO-3 (Orbiting Carbon Observatory 3) is a NASA carbon-monitoring instrument deployed on the International Space Station in May 2019, attached to the Japanese Experiment Module Exposed Facility (JEM-EF).[1][2]

OCO-3 shares the same three-channel grating spectrometer design as OCO-2, covering the oxygen A-band, the weak CO2 band, and the strong CO2 band. The spacecraft carries a Pointing Mirror Assembly (PMA) that enables two observing modes beyond the nadir-only geometry of OCO-2: Target Mode, which tracks a specific surface site across the overpass, and Snapshot Area Map (SAM) mode, which collects hundreds to thousands of SIF retrievals across a 80x80 km area at biologically and ecologically diverse sites in a single pass.[1]

Because OCO-3 orbits on the ISS at 408 km altitude and 51.6-degree inclination, it observes at varying times of day rather than at the fixed sun-synchronous crossing time of OCO-2. This variable local solar time sampling provides a different temporal context for CO2 and SIF measurements compared to sun-synchronous orbits with fixed crossing times. Sun-induced fluorescence retrieval at 757 nm and 740 nm has been demonstrated from OCO-3 data.[2]

Where this fits, supply chain

Compositional position

OCO-2 (Orbiting Carbon Observatory 2) ——— this successor
Sources
Cite https://eo-atlas.org/missions/oco-3 Markdown twin → Field definitions →