Revised historical solar irradiance forcing

作者：‪Tatiana Egorova, W. Schmütz, Eugene Rozanov, A. I. Shapiro, Ilya Usoskin, J. Beer, R. V. Tagirov, Thomas Peter · 发表于：Springer Link (Chiba Institute of Technology) · 年份：2018 · DOI：10.1051/0004-6361/201731199/pdf · 被引用次数：78 · 研究领域：Solar and Space Plasma Dynamics、Solar Radiation and Photovoltaics、Geophysics and Gravity Measurements

Context: There is no consensus on the amplitude of historical solar forcing. The estimated magnitude of the total solar irradiance (TSI) difference between the Maunder minimum and the present time ranges from 0.1 to 6 W m⁻² making the simulation of the past and future climate uncertain. One reason for this disagreement is the applied evolution of the quiet Sun brightness in 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 for the solar irradiance variability on decadal to millennial timescales. Methods: The spectral solar irradiance (SSI) is calculated as a weighted sum of the contributions from sunspot umbra, sunspot penumbra, faculae, and quiet Sun, which are pre-calculated with the NLTE Spectral SYnthesis code (NESSY). We introduce activity belts of the contributions from sunspots and faculae and a new structure model for the quietest state of the Sun. We assume that the brightness of the quiet Sun varies in time proportionally to the secular (22-yr smoothed) variation of the solar modulation potential. Results: A new reconstruction of the TSI and SSI covering the period 6000 BCE – 2015 CE is presented. The model simulates solar irradiance variability during the satellite era well. The TSI change between the Maunder and recent minima ranges between 3.7 and 4.5 W m⁻² depending on the applied solar modu...