Projections of the hydrogen column density, N_H, employing purely advective CR transport. The panels show the x−z plane of a section extending from z=0 to z=2H and the depth of the projection is 1 H. The snapshot is at t=7 t_cool≈2 t_ff. All simulations were initialised with different relative CR pressure, X_{cr, 0}. The density of the clouds decreases with increasing CR pressure, while the cloud size increases. In the CR pressure dominated run with X_{cr, 0}=3, cold gas condensation is entirely suppressed. This illustrates that advective CRs alter the morphology of the CGM significantly and suppress the formation of cold clouds.