Please use this identifier to cite or link to this item: https://doi.org/10.21256/zhaw-4656
Title: Implications of potential future grand solar minimum for ozone layer and climate
Authors : Arsenovic, Pavle
Rozanov, Eugene
Anet, Julien
Stenke, Andrea
Schmutz, Werner
Peter, Thomas
Published in : Atmospheric Chemistry and Physics
Volume(Issue) : 18
Pages : 3469
Pages to: 3483
Publisher / Ed. Institution : Copernicus
Issue Date: 2018
License (according to publishing contract) : CC BY 4.0: Namensnennung 4.0 International
Type of review: Open peer review
Language : English
Subject (DDC) : 500: Natural sciences and mathematics
Abstract: Continued anthropogenic greenhouse gas (GHG) emissions are expected to cause further global warming throughout the 21st century. Understanding the role of natural forcings and their influence on global warming is thus of great interest. Here we investigate the impact of a recently proposed 21st century grand solar minimum on atmospheric chemistry and climate using the SOCOL3-MPIOM chemistry–climate model with an interactive ocean element. We examine five model simulations for the period 2000–2199, following the greenhouse gas concentration scenario RCP4.5 and a range of different solar forcings. The reference simulation is forced by perpetual repetition of solar cycle 23 until the year 2199. This reference is compared with grand solar minimum simulations, assuming a strong decline in solar activity of 3.5 and 6.5Wm−2, respectively, that last either until 2199 or recover in the 22nd century. Decreased solar activity by 6.5Wm−2 is found to yield up to a doubling of the GHG-induced stratospheric and mesospheric cooling. Under the grand solar minimum scenario, tropospheric temperatures are also projected to decrease compared to the reference. On the global scale a reduced solar forcing compensates for at most 15% of the expected greenhouse warming at the end of the 21st and around 25% at the end of the 22nd century. The regional effects are predicted to be significant, in particular in northern high-latitude winter. In the stratosphere, the reduction of around 15% of incoming ultraviolet radiation leads to a decrease in ozone production by up to 8%, which overcompensates for the anticipated ozone increase due to reduced stratospheric temperatures and an acceleration of the Brewer–Dobson circulation. This, in turn, leads to a delay in total ozone column recovery from anthropogenic halogen-induced depletion, with a global ozone recovery to the pre-ozone hole values happening only upon completion of the grand solar minimum.
Departement: School of Engineering
Organisational Unit: Centre for Aviation (ZAV)
Publication type: Article in scientific Journal
DOI : 10.5194/acp-18-3469-2018
10.21256/zhaw-4656
ISSN: 1680-7324
URI: https://digitalcollection.zhaw.ch/handle/11475/8917
Appears in Collections:Publikationen School of Engineering

Files in This Item:
File Description SizeFormat 
2018_Anet_Implications_of_potential_future_grand_solar_minimum.pdf8.67 MBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.