  We investigate the scalar mode of perturbation of super inflation in the
version of loop quantum cosmology in which the gauge invariant holonomy
corrections are considered. Given a background solution, we calculate the power
spectrum of the perturbation in the classical and LQC conditions. Then we
compute the anisotropy originated from the perturbation. It is found that in
the presence of the gauge invariant holonomy corrections the power spectrum is
exponentially blue and the anisotropy also grows exponentially in the epoch of
super inflation.
