Author/Authors :
Barwick، نويسنده , , S.W. and Beatty، نويسنده , , J.J and Bower، نويسنده , , C.R and Chaput، نويسنده , , C. and Coutu، نويسنده , , S. and de Nolfo، نويسنده , , G. and Ellithorpe، نويسنده , , D. and Ficenec، نويسنده , , D. and Knapp، نويسنده , , J. and Lowder، نويسنده , , D.M and McKee، نويسنده , , S. and Müller، نويسنده , , D. and Musser، نويسنده , , J.A and Nutter، نويسنده , , S.L?. and Schneider، نويسنده , , E. and Swordy، نويسنده , , S.P. and Tang، نويسنده , , K.K and Tarlé، نويسنده , , G. and Tomasch، نويسنده , , A.D and Torbet، نويسنده , , E.، نويسنده ,
Abstract :
The HEAT (High-Energy Antimatter Telescope) instrument has been developed for a series of observations in cosmic-ray astrophysics that require the use of a superconducting magnet spectrometer. This paper describes the first configuration of HEAT which is optimized for the detection of cosmic-ray electrons and positrons below 100 GeV. In addition to the spectrometer, a combination of time-of-flight scintillators, a transition radiation detector, and an electromagnetic shower counter, provides particle identification, energy measurement, and powerful discrimination against the large background of protons. The instrument was successfully flown aboard high-altitude balloons in 1994 and 1995. The design and construction of the spectrometer and of the detector systems are described, and the performance of the instrument is demonstrated with data obtained in flight.
Keywords :
Cosmic rays , Magnet spectrometer , Positrons , Balloon instrumentation
