To mitigate the effects of climate change due to greenhouse gases (GHGs), it is vital that we understand the exchange of CO 2 between the atmosphere, biosphere, and ocean, and how these exchanges might vary with time. Previous studies have shown that the land biosphere is a substantial sink of atmospheric CO 2 at present (e.g., Ballantyne et al., 2012; Denning et al., 1995; Gurney et al., 2004; Tans et al., 1990), but much remains unknown about its precise magnitude and long-term trajectory, what accounts for its variability, and to what extent it is tropical or extratropical (Crowell et al., 2019; Schimel et al., 2015). In part, this lack of understanding is due to a gap in observational coverage at regional-to-continental scales (spatially, ∼10 3-10 4 km). While eddy flux towers can provide measurements of surface CO 2 fluxes at local scales (Luyssaert et al., 2007), and hemispheric-to-global fluxes can be constrained by mole fraction measurements at remote sites (Ciais et al., 2019), at intermediate scales neither method is completely satisfactory. Measurements of CO 2 mole fraction from in situ stations do not have a straightforward relationship to surface fluxes on intermediate scales (Stephens et al., 2007), and these stations are predominantly located in the mid-latitudes, limiting the assessment of surface fluxes in tropical and high-latitude regions (Peylin et al., 2013). The current state of the art method of generating a full atmospheric analysis of CO 2 mole fractions and surface fluxes on regional-to-global scales is through the use of global flux inversion models (