  This work is devoted to study the effects of Einstein-\AE ther gravity on the
dynamics of magnetized particles orbiting a static, spherically symmetric and
uncharged black hole immersed in an external asymptotically uniform magnetic
field in both comoving and proper observers frames. The analysis is carried out
by varying the free parameters $c_{13}$ and $c_{14}$ of the Einstein-\AE ther
theory and noticing their impacts on the particle trajectories, radii of the
innermost stable circular orbits (ISCOs), and the amount of center-of-mass
energy produced as a result of the collision. The strength of the magnetic
field and the location of circular orbits is significantly affected by varying
the above free parameters. We have also made detailed comparisons between the
effects of parameters of Einstein-\AE ther and spin of rotating Kerr black
holes on ISCO followed by magnetized particles and noticed that both black
holes depict similar behaviour for suitable values of $c_{13}$, $c_{14}$, spin
and the magnetic coupling parameters which provide exactly the same values for
the ISCO. Finally, we have analysed the cases when a static \AE ther black hole
can be described as Schwarzschild black hole in modified gravity (MOG) with the
corresponding values of the parameters of the black holes.
