Radial profiles of the rest-mass density ρ, the radial coordinate velocity ${\tilde{v}}^r$, the specific internal energy ε, and the radial component of the magnetic field B^r of the magnetized Bondi accretion test, performed without the energy-entropy switch. We show the results obtained with the MFV (orange triangles) and MFM mode (purple circles), at time t = 10M in the low-magnetization case. The exact solution is reported in each panel by a dashed black line.