Author/Authors :
Bidoli، نويسنده , , V. and Casolino، نويسنده , , M. and Pascale، نويسنده , , M.P.De and Morselli، نويسنده , , A. and Furano، نويسنده , , G. and Picozza، نويسنده , , P. and Scoscini، نويسنده , , A. and Sparvoli، نويسنده , , R. and Barbiellini، نويسنده , , G. and Bonvicini، نويسنده , , W. and Cirami، نويسنده , , R. and Schiavon، نويسنده , , P. and Vacchi، نويسنده , , A. and Zampa، نويسنده , , N. and Ambriola، نويسنده , , M. and Bello، نويسنده ,
Abstract :
In June 1998 the telescope NINA will be launched in space on board of the Russian satellite Resource-01 n.4. The main scientific objective of the mission is the study of the anomalous, galactic and solar components of the cosmic 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 beam at the GSI Laboratory in Germany in 1997; we report here on the results obtained during the beam calibration.
Keywords :
Cosmic rays , Isotopic composition , Satellite , Silicon detector , Beam test
