Fig. 8
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Quadrupole power ratios, P2/P0, versus the octupole power-ratios, P3/P0, of the total images of the different line emission in Kepler and Tycho. The dots represent the values measured for the pGMCA images obtained from the real data, and the error bars the standard deviation of fifty selected outputs from pGMCA on constrained bootstrap resamplings.
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