  We analyze the longitude-velocity diagram (LVD) of the CO-line emission from
archival data and use the most accurate rotation curve (RC) of the Milky Way to
transform radial velocity to face-on position in the Galactic plane. We point
out that the face-on transformation is highly sensitive to the adopted RC,
especially in the inner Milky Way, in the sense that deviations of the RC from
the true rotation velocity yield an artifact hole or overcrowded concentration
along the tangent circle for over- or under-estimated RC. Even if the RC is
sufficiently accurate, non-circular motion such as with the 3 kpc expanding
ring causes significant artifacts in the resulting face-on-map as long as a
circular rotation is assumed. On the other hand, if we properly take into
account the non-circular motion, it can be used to solve the near-far
degeneracy problem of determination of kinematic distance. We thus propose a
new method to solve the degeneracy by incorporating the expanding motion of a
ring or arms. We apply the method to the LVD of the 3-kpc expanding ring and
present its face-on map projected onto the galactic plane for the first time.
