In June 1998 the telescope NINA will be launched in space on board of the R
ussian satellite Resource-Ol n.4. The main scientific objective of the miss
ion is the study of the anomalous, galactic and solar components of the cos
mic rays in the energy interval 10-200 MeV/n. The core of the instrument is
a silicon detector whose performances have been tested with a particle bea
m at the GSI Laboratory in Germany in 1997; we report here on the results o
btained during the beam calibration. (C) 1999 Elsevier Science B.V. All rig
hts reserved.