Reconstructions of the total solar irradiance for the Holocene. The figure has the same structure as Fig. 5, but for the period 9495 BC to the present. See the caption of Fig. 5 for more information. While the green line in panel c) indicates the number of reconstructions employed to compute the uncertainty of the TSI due to the uncertainty of the evolution of the geomagnetic dipole moment, the black line represents the long-term trend of the uncertainty of the evolution of the geomagnetic dipole moment (y =  −1.7  ×  10 ⁻ 5 ∗ t + 0.15 [W/m²]). The period for which only VADM reconstructions are available is indicated in panel d).