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contributor authorCrooks, Simon A.
contributor authorGray, Lesley J.
date accessioned2017-06-09T17:00:25Z
date available2017-06-09T17:00:25Z
date copyright2005/04/01
date issued2005
identifier issn0894-8755
identifier otherams-77789.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4220385
description abstractA multiple linear regression analysis of the ERA-40 dataset for the period 1979?2001 has been used to study the influence of the 11-yr solar cycle on atmospheric temperature and zonal winds. Volcanic, North Atlantic Oscillation (NAO), ENSO, and quasi-biennial oscillation (QBO) signatures are also presented. The solar signal is shown to be readily distinguishable from the volcanic signal. The main solar signal is a statistically significant positive response (i.e., warmer in solar maximum) of 1.75 K over the equator with peak values at 43 km and a reversed signal of similar magnitude at high latitudes that is seasonally dependent. Consistent with this is a statistically significant zonal wind response of up to 6 m s?1 in the subtropical upper stratosphere/lower mesosphere that is also seasonally dependent. The wind anomalies are westerly/easterly in solar maximum/minimum. In addition, there is a statistically significant temperature response in the subtropical lower stratosphere that shows similarity in spatial structure to the QBO response, suggesting a possible interaction between the solar and QBO signals in this region. The solar response in tropospheric zonal winds is small but significant, confirming previous studies that indicate a possible modulation of the Hadley circulation.
publisherAmerican Meteorological Society
titleCharacterization of the 11-Year Solar Signal Using a Multiple Regression Analysis of the ERA-40 Dataset
typeJournal Paper
journal volume18
journal issue7
journal titleJournal of Climate
identifier doi10.1175/JCLI-3308.1
journal fristpage996
journal lastpage1015
treeJournal of Climate:;2005:;volume( 018 ):;issue: 007
contenttypeFulltext


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