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Fig. 6

image

Calibration of the -index by comparing the measured -index from HERMES with the average tabulated value from MWO-observations (cf. Table 6). For multiple observations, the vertical error bars reflect the scatter of those stars in the MWO catalogue, otherwise, the reported uncertainty was adopted. The red line depicts the linear correlation. For comparison, the instrumental -value of the Sun, measured in minimum phase of cycle 23 in August 2009 and in maximum phase of cycle 24 April 2015, on the horizontal axis is shown, reflecting the variation . The scatter of within the time series of our observations of Europa is shown with the blue symbol in the upper left part of the diagram.

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