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<div>Precise knowledge of sources and sinks in the carbon cycle is desired to understand its sensitivity to climate change, and to account and verify man-made emissions. An important role herein play extended sources like urban areas. While in-situ measurements of carbon dioxide (CO<sub>2</sub>)&#160;and&#160;methane&#160;(CH<sub>4</sub>) are highly accurate but localized, satellites measure column-integrated concentrations over an extended footprint. Our innovative measurement technique aims at determining CO<sub>2</sub> and CH<sub>4</sub> concentrations on the scale of a few kilometers near the ground, and therefore fills the sensitivity gap between in-situ and satellite measurements.</div>
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<div>Our development starts out from the EM27/SUN Fourier transform spectrometer, which is a reliable, mobile and commercially available spectrometer for the measurement of CO<sub>2</sub> and CH<sub>4</sub> column densities using direct sunlight spectra. We increased the radiometric sensitivity of the instrument by enhancing optical throughput and replacing the detector module by a thermoelectrically cooled detector. This enables the measurement of surface scattered sunlight spectra in the range of 4000 - 11000 cm<sup>-1</sup> under various viewing directions. Our setup is independent of sun position and exhibits a high sensitivity to the concentrations in the lower boundary layer, due to the near ground horizontal path component.</div>
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<div>Here, we report progress on our instrumental developments, as well as first retrievals of column averaged CO<sub>2</sub> and CH<sub>4</sub> mole fractions from ground-scattered sunlight spectra recorded with this setup. We present the instrument modifications and extensions to the experimental setup: A Lambertian reflector allows for reference measurements without horizontal path component, a coaligned camera enables specific targeting and the motorized tracking system facilitates automated alternation between multiple targets. We characterize the setup with a spectral resolution of 0.54 &#177; 0.03 cm<sup>-1</sup> a signal to noise ratio above 200 for solar zenith angles < 85&#176;, and precision of 1.8 ppm and 9 ppb regarding the inferred column averaged CO<sub>2</sub> and CH<sub>4</sub> mole fractions obtained from retrievals with a simple radiative transfer model, neglecting atmospheric scattering.</div>
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