The signal of the 11-year solar cycle in the global stratosphere

The search for a signal of the 11-year sunspot cycle in the heights and tem peratures of the lower stratosphere was previously successfully conducted f or the northern hemisphere with a data set from the Freie Universitat Berli n, covering four solar cycles. This work has been extended to the whole glo be by means of the NCEP/NCAR reanalyses for the period 1968-1996. The re-an alyses show that the signal exists in the southern hemisphere too, and that it is of nearly the same size and shape as on the northern hemisphere. The NCEP/NCAR reanalyses yield higher correlations with the solar cycle than d o the Berlin analyses for the same period, because the interannual variabil ity is lower in the NCEP/NCAR data. The correlations between the solar cycle and the zonally averaged temperatu res at the standard levels between 200 and 10 hPa are largest between the t ropopause and the 25 km level, that is, in the ozone layer. This may be par tly a direct effect in this layer? because of more absorber (ozone) and mor e ultraviolet radiation from the sun in the peaks of the 11-year solar cycl e. However, it is more likely to be mainly an indirect dynamical consequenc e of UV absorption by ozone in the middle and upper stratosphere. The largest temperature correlations move with the sun from one summer hemi sphere to the other, and the largest height correlations move poleward from winter to summer. (C) 1999 Elsevier Science Ltd. All rights reserved.