Evidence of the solar cycle in stratospheric polar temperature rests on a c
onnection to the quasi-biennial oscillation (QBO) of equatorial wind. New e
vidence reported here establishes a mechanism for how the solar signature i
n polar temperature follows from the QBO, which itself is shown to vary wit
h the solar cycle. Equatorial westerlies below 30 mb vary systematically wi
th solar activity, as do equatorial easterlies above 30 mb. Changes in thei
r duration introduce a systematic drift into the QBO's phase relative to wi
nter months, when the polar vortex is sensitive to equatorial wind. Corresp
onding changes in the polar-night vortex are consistent with the solar sign
ature observed in wintertime records of polar temperature that have been st
ratified according to the QBO.