  Energy loss in anisotropic hot dense QGP in external magnetic field is
studied within holographic approach. Energy loss is calculated by estimation of
behaviour of the spatial Wilson loops using the effective potential technique.
We examine the dependence of the effective potential on the spatial Wilson
loops orientation in fully anisotropic background. For this purpose we obtain
general formulas for the effective potential and study appearance of the
effective potential dynamical wall. We consider particular fully anisotropic
model [arXiv:2011.07023] supported by Einstein-Dilaton-three-Maxwell action.
The effective potential strongly depends on the parameters of anisotropy and
magnetic field, therefore the energy loss depends on physical parameters $-$
$T$, $\mu$, $c_B$ and orientation. Orientation is determined by angles between
the moving heavy quark velocity, the axis of heavy ions collision and their
impact parameter vector.
