  We present a numerical code, written in C, which can be used to simulate or
to analyze the emission of Blazars over the entire electromagnetic spectrum.
Our code can reproduce the following features: synchrotron emission, inverse
Compton emission (Thomson Klein-Nishina regime) external Compton emission,
accretion disk variability using a Cellular Automata algorithm, temporal
evolution of the emitting plasma energy distribution, flaring phenomena, light
curves in the rest and in the observer frame (taking account for time crossing
effects). In this paper we will show mainly the accretion disk simulation, and
the implications in the External Compton scenario.
