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Fig. 5 | Carbon Balance and Management

Fig. 5

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. 5

a Number of 8:30–11:30 time windows in a year for which the posterior uncertainty in the 3 h mean emissions are less than 20% (N20) in INV-3 h; b Relative posterior uncertainty in annual CO2 emissions in INV-annual for 1 satellite with a swath width of 300 km (blue) and for 2 satellites with a swath width of 150 km (purple); and c the same as b but for absolute values of posterior uncertainty. 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 in the bin and the fraction of total CO2 emissions generated by the clumps. Dots and error bars are the median and interquartile range of N20 (a) and posterior uncertainty (b)

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