  In this article, we examine the effects of anisotropy on a model of canonical
warm inflation with the power-law potential. The results of this model are
compared to Planck satellite observational data. Using a conventional local
scalar fi?eld in the Bianchi type I metric, the slow-roll conditions and the
suitable regions, where the free parameters of the model show a good agreement
with Planck results, are investigated in detail. Following the usual
calculations for warm inflationary approaches, the early universe in two
different dissipative regimes, namely the weak dissipative and the strong
dissipative ones, is investigated. In this regard, the slow-roll parameters and
their observational indices in both regimes are obtained and finally, it is
shown that this model is in good agreement with observatio
