A demonstration of how changing the parameters of the planar reversal model adjusts the simulated ﹩{{\rm{M1}}}_{{{\rm{screen}}}_{{\rm{rev}}}}﹩ profiles for Galactic latitude b = 30°. Red and blue shading are included for quick visual identification of the positive and negative peaks. (a) Varying the path length, R, shifts the longitude of the zeros (circles) and peaks (squares) horizontally. (b) Varying the vertical tilt angles, β_CW and β_CCW, shifts the profiles vertically.