The INTEGRAL gamma-ray spectrometer SPI being a system of 19 HPGe detectors
combined with a coded mask aperture will provide sky images. In order to m
ake possible the deconvolution of these images, the response of the detecti
on plane must be well known. A first experiment of a single detector effici
ency mapping revealed great variations. Then it is clear that a detailed st
udy of the local efficiency of the detectors as a function of position and
angle of incident photons is needed. In this paper we present a setup allow
ing such studies. Performance and limitations of this mapping system are pr
esented, illustrated by the first results obtained for one SPI detector. We
present also results of the Monte Carlo simulation of the experiment.