Abstract. Several single-platform satellite missions have been
designed during the past decades in order to retrieve the atmospheric
concentrations of anthropogenic greenhouse gases (GHG), initiating worldwide
efforts towards better monitoring of their sources and sinks. To set up a
future operational system for anthropogenic GHG emission monitoring, both
revisit frequency and spatial resolution need to be improved. The Space
Carbon Observatory (SCARBO) project aims at significantly increasing the
revisit frequency of spaceborne GHG measurements, while reaching
state-of-the-art precision requirements, by implementing a concept of small
satellite constellation. It would accommodate a miniaturised GHG sensor
named NanoCarb coupled with an aerosol instrument, the multi-angle
polarimeter SPEXone. More specifically, the NanoCarb sensor is a static
Fabry–Pérot imaging interferometer with a 2.3×2.3 km2 spatial resolution and 200 km swath. It samples a truncated interferogram at optical path differences (OPDs) optimally sensitive to all the geophysical parameters necessary to retrieve column-averaged dry-air mole fractions of CO2 and CH4 (hereafter XCO2 and XCH4).
In this work, we present the Level 2 performance assessment of the concept proposed in the SCARBO project. We perform inverse radiative transfer to retrieve XCO2 and XCH4 directly from synthetic NanoCarb truncated interferograms and provide their systematic and random errors, column vertical sensitivities, and degrees of freedom as a function of five
scattering-error-critical atmospheric and observational parameters. We show
that NanoCarb XCO2 and XCH4 systematic retrieval errors can be greatly reduced with SPEXone posterior outputs used as improved prior
aerosol constraints. For two-thirds of the soundings, located at the centre
of the 200 km NanoCarb swath, XCO2 and XCH4 random errors span 0.5–1 ppm and 4–6 ppb, respectively, compliant with their respective 1 ppm
and 6 ppb precision objectives. Finally, these Level 2 performance results
are parameterised as a function of the explored scattering-error-critical
atmospheric and observational parameters in order to time-efficiently
compute extensive L2 error maps for future CO2 and CH4 flux
estimation performance studies.