首页    期刊浏览 2024年12月11日 星期三
登录注册

文章基本信息

  • 标题:Revised historical solar irradiance forcing
  • 本地全文:下载
  • 作者:T. Egorova ; W. Schmutz ; E. Rozanov
  • 期刊名称:Astronomy & Astrophysics
  • 印刷版ISSN:0004-6361
  • 电子版ISSN:1432-0746
  • 出版年度:2018
  • 卷号:615
  • DOI:10.1051/0004-6361/201731199
  • 语种:English
  • 出版社:EDP Sciences
  • 摘要: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−2making 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−2depending on the applied solar modulation potential. The implementation of a new quietest Sun model reduces, by approximately a factor of two, the relative solar forcing compared to the largest previous estimation, while the application of an updated solar modulation potential increases the forcing difference between the Maunder minimum and the present by 25–40%.
  • 关键词:Key wordsensolar-terrestrial relationsSun: UV radiationSun: atmosphereradiative transferline: formationSun: faculae, plages
国家哲学社会科学文献中心版权所有