Eleven-year solar cycle variations in the atmosphere: observations, mechanisms and models.

Labitzke, K. and Matthes, Katja (2003) Eleven-year solar cycle variations in the atmosphere: observations, mechanisms and models. Holocene, 13 (3). pp. 311-317. DOI 10.1191/0959683603hl623rp.

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Abstract

The understanding of natural and anthropogenic climatic change is an important issue in recent studies. The influence of the Sun (11-year solar cycle) as a natural variability factor on the atmosphere is discussed. Statistical studies with observational data (NCEP/NCAR re-analyses) covering four solar cycles show high correlations between the 11 -year solar signal and meteorological parameters, e.g., the geopotential heights and temperatures, in the lower stratosphere and troposphere. Studies with general circulation models (GCM) have discussed the possibility of an indirect dynamical response to direct changes in solar irradiance and ozone in the stratosphere. A physical mechanism explaining the solar influence on the atmosphere is still missing. Part of the mechanism understood so far and ideas from model and observational studies are presented.

Document Type: Article
Keywords: numerical modelling experiments; solar cycle; climatic change; mechanisms; observational data; meteorological parameters; Sun; NORTHERN-HEMISPHERE WINTER; STRATOSPHERIC CIRCULATION; INTERANNUAL VARIABILITY; IRRADIANCE VARIATIONS; CLIMATE-CHANGE; QBO; TROPOSPHERE; OZONE; ULTRAVIOLET; CONNECTION
Refereed: Yes
Open Access Journal?: No
Publisher: Sage Publishing
Date Deposited: 02 Aug 2012 13:13
Last Modified: 29 Jul 2020 12:54
URI: https://oceanrep.geomar.de/id/eprint/14974

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