  In this paper we present our point of view on correct physical interpretation
of the Bel-Robinson tensor within the framework of the standard General
Relativity ({\bf GR}), i.e., within the framework of the {\bf GR} without
supplementary elements like arbitrary vector field, distinguished tetrads field
or second metric. We show that this tensor arises as a consequence of the
Bianchi identities and, in a natural manner, it is linked to the differences of
the canonical gravitational energy-momentum calculated in normal coordinates
{\bf NC(P)}.
