Revised historical solar irradiance forcing
T. Egorova, W. Schmutz, E. Rozanov, A. I. Shapiro, I. Usoskin, J., Beer, R. V. Tagirov, and T. Peter

TL;DR
This study presents a new reconstruction of solar irradiance variability from 6000 BCE to 2015 CE, highlighting the impact of quiet Sun models and magnetic activity proxies on estimated solar forcing.
Contribution
It introduces a novel quiet Sun model and incorporates updated solar magnetic activity proxies, refining the estimates of historical solar irradiance changes.
Findings
TSI change between Maunder minimum and recent minima ranges from 3.7 to 4.5 W/m2.
Implementation of a new quiet Sun model reduces relative solar forcing by about half.
Updated solar modulation potential increases the forcing difference by 25-40%.
Abstract
Context. There is no consensus on the amplitude of the historical solar forcing. The estimated magnitude of the total solar irradiance difference between Maunder minimum and present time ranges from 0.1 to 6 W/m2 making uncertain the simulation of the past and future climate. One reason for this disagreement is the applied evolution of the quiet Sun brightness in the solar irradiance reconstruction models. This work addresses the role of the quiet Sun model choice and updated solar magnetic activity proxies on the solar forcing reconstruction. Aims. We aim to establish a plausible range of the solar irradiance variability on decadal to millennial time scales. Methods. The spectral solar irradiance (SSI) is calculated as a weighted sum of the contributions from sunspot umbra/penumbra, fac- ulae and quiet Sun, which are pre-calculated with the spectral synthesis code NESSY. We introduce…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
