  In this paper we investigate the induced inflation with two flat regions: one
Starobinsky-like plateau in big field regime and one shorter plateau around the
saddle point of the Einstein frame potential. This multi-phase inflationary
scenario can be used to solve the problem of classical cosmology. The inflation
at the saddle-point plateau is consistent with the data and can have
arbitrarily low scale. The results can be useful in the context of the
Higgs-Axion relaxation and in a certain limit they are equivalent to the
$\alpha$-attractors.
