Impact of a potential 21st century "grand solar minimum" on surface temperatures and stratospheric ozone
We investigate the effects of a recently proposed 21st century Dalton minimum like decline of solar activity on the evolution of Earth's climate and ozone layer. Three sets of two member ensemble simulations, radiatively forced by a midlevel emission scenario (Intergovernmental Panel on Climate...
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Published in: | Geophysical research letters Vol. 40; no. 16; pp. 4420 - 4425 |
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Main Authors: | , , , , , , , , , , |
Format: | Journal Article |
Language: | English |
Published: |
Washington, DC
Blackwell Publishing Ltd
28-08-2013
American Geophysical Union John Wiley & Sons, Inc |
Subjects: | |
Online Access: | Get full text |
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Summary: | We investigate the effects of a recently proposed 21st century Dalton minimum like decline of solar activity on the evolution of Earth's climate and ozone layer. Three sets of two member ensemble simulations, radiatively forced by a midlevel emission scenario (Intergovernmental Panel on Climate Change RCP4.5), are performed with the atmosphere‐ocean chemistry‐climate model AOCCM SOCOL3‐MPIOM, one with constant solar activity, the other two with reduced solar activity and different strength of the solar irradiance forcing. A future grand solar minimum will reduce the global mean surface warming of 2 K between 1986–2005 and 2081–2100 by 0.2 to 0.3 K. Furthermore, the decrease in solar UV radiation leads to a significant delay of stratospheric ozone recovery by 10 years and longer. Therefore, the effects of a solar activity minimum, should it occur, may interfere with international efforts for the protection of global climate and the ozone layer.
Key Points
A future grand solar minimum will modify the global ozone distribution
A future grand solar minimum will have an impact on the rate of global warming
Strength and duration of a future grand solar minimum are highly uncertain |
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Bibliography: | Supporting informationSupporting informationSupporting informationSupporting informationSupporting informationSupporting informationSupporting information ark:/67375/WNG-JDD0VR75-W ArticleID:GRL50806 istex:28F5FA0F87294A32690921E2062FDD772BE40A80 ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 23 |
ISSN: | 0094-8276 1944-8007 |
DOI: | 10.1002/grl.50806 |