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Fig. 2 | Carbon Balance and Management

Fig. 2

From: The potential of a constellation of low earth orbit satellite imagers to monitor worldwide fossil fuel CO2 emissions from large cities and point sources

Fig. 2

Number of 8:30–11:30 time windows in a year (here for the year 2008) for which the posterior uncertainty in the 3 h mean emissions are less than 20% (N20) in INV-3 h. The results are binned according to the clump annual emission with bin limits given on the x-axis of the figure. Numbers within the figure indicate the number of clumps and the fraction of total CO2 emissions generated from all the clumps within each bin. Dots and error bars are the median and interquartile range of N20

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