  This article completes and extends a recent study of the Grad-Shafranov (GS)
reconstruction in toroidal geometry, as applied to a two and a half dimensional
configurations in space plasmas with rotational symmetry. A further application
to the benchmark study of an analytic solution to the toroidal GS equation with
added noise shows deviations in the reconstructed geometry of the flux rope
configuration, characterized by the orientation of the rotation axis, the major
radius, and the impact parameter. On the other hand, the physical properties of
the flux rope, including the axial field strength, and the toroidal and
poloidal magnetic flux, agree between the numerical and exact GS solutions. We
also present a real event study of a magnetic cloud flux rope from \textit{in
situ} spacecraft measurements. The devised procedures for toroidal GS
reconstruction are successfully executed. Various geometrical and physical
parameters are obtained with associated uncertainty estimates. The overall
configuration of the flux rope from the GS reconstruction is compared with the
corresponding morphological reconstruction based on white-light images. The
results show overall consistency, but also discrepancy in that the inclination
angle of the flux rope central axis with respect to the ecliptic plane differs
by about 20-30 degrees in the plane of the sky. We also compare the results
with the original straight-cylinder GS reconstruction and discuss our findings.
