A toy disc model with advection dominated accretion on to a black hole is presented. The advection dominated accretion flows (ADAFs) are assumed to exist in the inner thick disc with rin ＜ r ＜ rout, and the disc is assumed to be geometrically thin for r ＞ rout. Compared with Paczynskis toy model the thick disc is not limited to be 100% advective. It tus out that the inner radius rin depends not only on the outer radius rout but also on the ADAF parameters f and ε. The effects of the inner thick disc on the radiation efficiency and the temperature profile of the outer thin disc are discussed in details.