  We present preliminary results on the possible effects that primordial
magnetic fields can have for a warm inflation scenario, based on global
supersymmetry, with a new-inflation-type potential. This work is motivated by
two considerations: first, magnetic fields seem to be present in the universe
on all scales, which rises the possibility that they could also permeate the
early universe; second, the recent emergence of inflationary models where the
inflaton is not assumed to be isolated but instead it is taken as an
interacting field, even during the inflationary expansion. The effects of
magnetic fields are included resorting to Schwinger proper time method.
