Time-averaged GRRT decomposed images with a black hole spin of a = 0.9375 at 230 GHz with a 163° inclination angle. From top to bottom: images using the R − β model with R_h = 1, the turbulent heating model, and the reconnection heating model, respectively. From left to right, the emissions come from every region: the whole region is depicted first, then the midplane, the nearside jet, and the farside jet, respectively. The eDF of all of the images is variable κ and the time-averaged total flux is 0.5 Jy at 230 GHz from t = 14 000 to 15 000 M.