Figure 12.
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Excerpt of four solar proxies, and their reconstruction with the 10.7 cm flux only, and with both the 10.7 and 30 cm fluxes. From top to bottom: the DSA, the MPSI, the MgII index, and the intensity of the H I line in (mW/m2/nm). The time interval is identical to that used in Figure 7.
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