  We study effect of superhorizon tensor perturbations on scalar perturbations,
so called effect of clustering fossils, in cosmological model in which
inflation is driven by both solid matter and scalar field. The effect deforms
primordial scalar power spectrum causing asymmetry in it, which leaves imprint
on CMB anisotropies and the cosmic structure. Parameter space of this combined
model allows for enhancement of logarithmic scale dependence of this
deformation, as opposed to simpler models in which such scale dependence is
suppressed by slow-roll parameters.
