It is shown that, using a pulsed laser to generate a laser guide star (LGS)
, a frame transfer technique at the focal plane of an auxiliary telescope c
an be used to retrieve the bidimensional tilt of such an LGS. We discuss ho
w this approach can be used to reduce from two to one the number of auxilia
ry telescopes in the NGS-based perspective technique proposed in the litera
ture. A discussion of the requirements for the laser pulse format is given.