The multiblackbody "SelfIrRadiated Funnel" model is designed to model opticallythick outflowdominated accretion. The basic idea is simple: you just assume a lot of matter, angular momentum and energy emerges in a limited volume. Momentum conservation leads to nonsphericity of the flow that has subsequently conical (funnellike) shape. The model calculates temperature distribution at the funnel walls (taking into account irradiation by iterative process) and the outer photosphere. We also assume that inside the cone there is a deep pseudophotosphere. Relativistic boosts are taken into account for high velocities. For a comprehensive description of the physical model, see: Abolmasov, P., Karpov, S. and Kotani, T. PASJ, 61, 2, 213.
par1 
tin, inner temperature (at the inner, insidethefunnel photosphere). 
par2 
rin, inner (insidethefunnel photosphere) radius in "spherisation radius" units (the latter is defined as 3 Κ Mdot / Ω_{f} c). 
par3 
rout, outer photosphere radius in "spherisation radius" units. 
par4 
theta, halfopening angle of the cone. 
par5 
incl, inclination angle of the funnel. Affects mainly selfoccultation and relativistic boost effects. 
par6 
valpha, velocity law exponent, v goes as r^{valpha}. 
par7 
gamma, adiabatic index. It affects the inner, hotter parts of the flow, therefore we set is to 4/3 by default. 
par8 
mdot, mass ejection rate in Eddington (critical) units. 
par9 
irrad, number of iterations for irradiation. 
norm 
