  The total spacetime manifold for a Schwarzschild black hole (BH) is described
by the Kruskal coordinates u=u(r,t) and v=v(r,t), where r and t are the
conventional Schwarzschild radial and time coordinates respectively. The
relationship between r and t for a test particle moving on a radial or
non-radial geodesic is well known. Similarly, the expression for the vacuum
Schwarzschild derivative for a geodesic, in terms of the constants of motion,
is well known. However, the same is not true for the Kruskal coordinates. Here,
we, first, explicitly obtain the value of the Kruskal coordinates on the Event
Horizon as a function of the constant of motion (E=energy per unit rest mass)
for a test particle on a radial geodesic by directly using the r-t relationship
as obtained by Chandrasekhar and also by Misner, Thorne and Wheeler. It is
found that u_H and v_H are finite for E <1. And then, we derive here the
expression for the Kruskal derivative for a radial geodesic in terms of the
constants of motion. In particular, it is seen that the value of |du/dv| (= 1)
is regular on the Event Horizon of the Black Hole. The regular nature of the
Kruskal derivative is in sharp contrast with the Schwarzschild derivative,
|dt/dr| =infty, at the Event Horizon.
