  In the present work warm inflationary universe model with viscous pressure on
the brane in high-dissipation regime is studied. We derive a condition which is
required for this model to be realizable in slow-roll approximation. We also
present analytic expressions for density perturbation and amplitude of tensor
perturbation in longitudinal gauge. General expressions of tensor-to-scalar
ratio, scalar spectral index and its running are obtained. We develop our model
by using chaotic potential, the characteristics of this model are calculated
for two specific cases: 1- Dissipative parameter $\Gamma$ and bulk viscous
parameter $\zeta$ are constant parameters. 2- Dissipative parameter as a
function of scalar field $\phi$ and bulk viscous parameter as a function of
radiation-matter mixture energy density $\rho$. The parameters of the model are
restricted by WMAP9, Planck and BICEP2 observational data.
