The emergence of the solar activity from the MM in the “recovery phase”. The black line gives the monthly means, R_G, of daily group sunspot numbers by Vaquero et al. (2016): note that values are only given for months in which more than 15 days of observations were available. The green line shows monthly mean of the near-Earth interplanetary magnetic field, B_IMF, derived by McCracken & Beer (2015) from the ¹⁰Be cosmogenic isotope abundances from the Dye-3 ice-core and North Greenland Ice Core Project (NGRIP), both from Greenland (Beer et al., 1998; Berggren et al., 2009): the black dashed line is the same data passed through a 1-4-6-4-1 filter. The blue line gives annual means of the heliospheric modulation potential, Φ_mod, derived from both the ¹⁴C and ¹⁰Be cosmogenic isotopes: the surrounding area gives the 2-sigma uncertainty band (Muscheler et al., 2007). The mauve line is the open solar flux, F_S, modelled by Lockwood & Owens (2014) from sunspot numbers. The vertical cyan and orange lines mark the times of the 1706 and 1715 eclipses, respectively.