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This paper explores the dynamics of warm intermediate and logamediateinflationary models during weak dissipative regime with a general form ofdissipative coefficient. We analyze these models within the framework oflocally rotationally symmetric Bianchi type I universe. In both cases, weevaluate solution of inflaton, effective scalar potential, dissipativecoefficient, slow-roll parameters, scalar and tensor power spectra, scalarspectral index and tensor to scalar ratio under slow-roll approximation. Weconstrain the model parameters using recent data and conclude that anisotropicinflationary universe model with generalized dissipation coefficient remainscompatible with WMAP9, Planck and BICEP2 data.

Inflationary Weak Anisotropic Model with General Dissipation Coefficient