Abstract
Numerical simulations are performed of the approach to the singularity in Gowdy spacetimes on ${S}^{2}\ifmmode\times\else\texttimes\fi{}{S}^{1}\ifmmode\times\else\texttimes\fi{}R$. The behavior is similar to that of Gowdy spacetimes on ${T}^{3}\ifmmode\times\else\texttimes\fi{}R$. In particular, the singularity is asymptotically velocity term dominated, except at isolated points where spiky features develop.
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