How large were the past changes in the sun?

We only have direct observations of total solar irradiance (TSI) since the beginning of the satellite era and substantial evidence for variations in the level of solar activity (from cosmogenic isotopes or sunspot records) in the past. Tying those factors together in order to estimate solar irradiance variations in the past is crucial for attributing past climate changes, particularly in the pre-industrial.

In the May issue of Astronomy & Astrophysics, Shapiro et al. present a new long-term reconstruction of the solar irradiance that implies much greater variation over the last 7000 years than any previously reconstruction. What is the basis for this difference?

Their results do not deviate much from previous work when it comes to the most recent period with modern instrumental observations, but Shapiro et al. obtain substantially lower radiance during the Maunder minimum than previous estimates.

Figure 1. TSI reconstructions from Schmidt et al (2011) with the new Shapiro et al (SEA) values all scaled to the same values in the last 30 years.

Shapiro et al estimate the total solar irradiance (TSI) during the Maunder minimum to be about 6 W/m2 less than at present, and hence the solar radiative forcing difference of about 1 W/m2. For comparison, the corresponding radiative forcing in the most recent IPCC report, however, ranges between +0.38 and +0.68 W/m2

How good are the new estimates? A major weakness of all such estimates – and Shapiro et al. is no different – is that the results cannot be tested on the basis of the last 30 years of solar observations. The paper is candid about this issue, and explains that this is partly because the time scale, on which their analysis rests, is 22 years. In any reconstruction, part of the analysis involves determining the degree which “magnetically enhanced contribution” contributes to the irradiance of the present “quiet sun”. These estimates were then scaled with the proxies for levels representing “quiet” sun activity.

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