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There was an omission which led to a discrepancy in the text about the scaling of the solar cycle component that was used.
Equation 4 in the originally published article was that suggested by Hoyt and Schatten (1993, HS93, hereafter) for scaling the solar cycle component. However, our analysis in Section 3.1 in the originally published article revealed that utilizing Equation 4 for scaling the solar cycle component resulted in amplifying the solar cycle variations compared to the original HS93 Total Solar Irradiance (TSI) series (see Figures 1 and 2). Consequently, we used an adjusted scaling factor by dividing it further by 1.5, resulting in a better reproduction of the original HS93 TSI series with their data as shown in Figure 7 of the originally published article. Thus, the actual scaling we used for the solar cycle component when reproducing the HS93 TSI series with their own data was
where ISNv1 is version 1 of the International Sunspot Number series.
To maintain consistency with the original HS93 TSI series, the same scaling for the solar cycle component was used in our update (taking into account the different reference level of ISNv1 and ISNv2 which requires a multiplication factor of 0.6, although potentially a factor of 0.7 would have been better to roughly account also for the Waldmeier discontinuity). Therefore, whenever we mention Equation 5 in Section 3 of the originally published article the actual equation that was used is
Unfortunately, this was not explicitly stated in the originally published article.
Furthermore, Equation 5 in the originally published article mistakenly reflected the reduced scaling shown in Equation 1 here and not the actual scaling between ISNv2 and PMOD (named after Physikalisch-Meteorologisches Observatorium Davos) TSI series. The correct scalings between ISNv2 and PMOD, ACRIM (Active Cavity Radiometer Irradiance Monitor), ROB (named after Royal Observatory of Belgium), and Montillet et al. (2022) TSI composites are 0.0056, 0.0064, 0.007, and 0.0062, respectively. The scalings are calculated based on annual means, which are derived from monthly means computed only for the overlapping days between each set of two series. Our suggested scaling is that determined with the Montillet et al. (2022) TSI composite, namely
We also stress that since this is just a scaling of the solar cycle component, it only affects the overall amplitude of solar cycles, while it does not affect the long-term trend of the reconstructions and, thus, any of the arguments made in the originally published article (see Figure 1). However, such greater solar cycle variations lead to a slightly worse agreement between our updated TSI series with the HS93 model and Earth’s temperatures (Table 2) further strengthening our conclusions. We do not change the figures and tables in the article since what is presented there is consistent with HS93. However, we consider as a more accurate update of the HS93 TSI series the one using Equation 3 to scale the solar cycle component.
For completeness, we add here the figures (Figures 2 – 7) and tables (Tables 1 – 2) that change if the solar cycle component was derived from Equation 4 (that suggested by HS93) as presented in the originally published article and Equation 3 when replicating the original HS93 series and creating our update, respectively. Figures from the originally published article that are not included here are not affected at all by this inconsistency.
References
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Chatzistergos, T. Correction to: A Discussion of Implausible Total Solar Irradiance Variations Since 1700. Sol Phys 299, 59 (2024). https://doi.org/10.1007/s11207-024-02308-9
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DOI: https://doi.org/10.1007/s11207-024-02308-9