The new PNe discovered in the Galactic bulge region by Boumis et. al. (2003, 2006), were studied in detail, using the photo—ionization model CLOUDY. Applying the imaging and spectroscopic results to the CLOUDY model, we determined the physical parameters and abundances of these PNe (like Te, ne, Tc, Lc etc). Their distance was also determined using statistical methods.