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Column abundances of carbon dioxide and methane retrieved from ground-based near-infrared solar spectra

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Figure

Figure 2.1. (a) Photograph of the automated FTS laboratory, located 25 m south of the WLEF Tall Tower
Figure 2.2. (a) A single spectrum recorded on 9 Sep 2004, with 0.014 cm absorptions by Hnoise ratio is ~900 for the InGaAs detector and ~500 for the Si diode detector
Figure 2.3. (a) Relationship between retrieved column O 2 and dry surface pressure for spectra recorded at airmasses between 2 and 3
Table 2.1.  Mean and standard deviation of column CO2 measurements during a one-hour observational period around local noon
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