  We use the publicly available code CMBFAST as modified by L. Pogosian and T.
Vachaspati to simulate the effects of wiggly cosmic strings on the Cosmic
Microwave Background (CMB). Using the modified CMBFAST code which takes into
account vector modes and models wiggly cosmic strings by the one scale model,
we go beyond the angular power spectrum to construct CMB temperature maps with
resolution of a few degrees. The statistics of these maps are then studied
using conventional and recently proposed statistical tests optimized for the
detection of hidden temperature discontinuities induced by the
Gott-Kaiser-Stebbins effect. We show however, that these realistic maps can not
be distinguished in a statistically significant way from purely Gaussian maps
with identical power spectrum.
