Time-averaged GRRT decomposed images at 86 (top) and 43 GHz (bottom) with a black hole spin of a = 0.9375 using the reconnection heating model with an inclination angle of 163°. From left to right, the emissions come from every region: the whole region is depicted first, then the midplane, the nearside jet, and farside jet, respectively. The eDF of all of the images used is variable κ and the time-averaged total flux is 0.5 Jy at 230 GHz from t = 14 000 to 15 000 M.