  The "fully charged" spin-2 field solution is presented. This is an analog of
the Coulomb solution in electrodynamics and represents the "non-waving" part of
the spin-2 field theory. Basic facts and definitions of the spin--2 field and
conformal Yano-Killing tensors are introduced. Application of those two objects
provides a precise definition of quasi-local gravitational charge. Next, the
3+1 decomposition leads to the construction of the momentary gravitational
charges on initial surface which is applicable for Schwarzschild-like
spacetimes.
