  This work presents a reduced chi^2_nu test to search for non-gaussian signals
in the CMBR TT power spectrum of recent CMBR data, WMAP, ACBAR and CBI data
sets, assuming a mixed density field including adiabatic and isocurvature
fluctuations. We assume a skew positive mixed model with adiabatic inflation
perturbations plus additional isocurvature perturbations possibly produced by
topological defects. The joint probability distribution used in this context is
a weighted combination of Gaussian and non-Gaussian random fields. Results from
simulations of CMBR temperature for the mixed field show a distinct signature
in CMB power spectrum for very small deviations (~ 0.1%) from a pure Gaussian
field, and can be used as a direct test for the nature of primordial
fluctuations. A reduced chi^2_nu test applied on the most recent CMBR
observations reveals that an isocurvature fluctuations field is not ruled out
and indeed permits a very good description for a flat geometry Lambda-CDM
universe, chi^2_930 ~ 1.5, rather than the simple inflationary standard model
with chi^2_930 ~ 2.3. This result may looks is particular discrepant with the
reduced chi^2 of 1.07 obtained with the same model in Spergel et al. (2003) for
temperature only, however, our work is restricted to a region of the parameter
space that does not include the best fit model for TT only of Spergel et al.
(2003).
