Title of article
The Cosmic Ray Energetics And Mass (CREAM) instrument
Author/Authors
Ahn، نويسنده , , H.S. and Allison، نويسنده , , P. and Bagliesi، نويسنده , , M.G. and Beatty، نويسنده , , J.J. and Bigongiari، نويسنده , , G. and Boyle، نويسنده , , P. and Childers، نويسنده , , J.T. and Conklin، نويسنده , , N.B. and Coutu، نويسنده , , S. and Duvernois، نويسنده , , M.A. and Ganel، نويسنده , , O. H. Han، نويسنده , , J.H. and Jeon، نويسنده , , J.A. and Kim، نويسنده , , K.C. and Lee، نويسنده , , J.K. and Lee، نويسنده , , M.H. and Lutz، نويسنده , , L. and Maestro، نويسنده , , P. and Malinin، نويسنده , , A. and Marrocchesi، نويسنده , , P.S. and Minnick، نويسنده , , S.A. and Mognet، نويسنده , , S.I. and Nam، نويسنده , , S.W. and Nutter، نويسنده , , S.L. and Park، نويسنده , , I.H. and Park، نويسنده , , N.H. and Seo، نويسنده , , E.S. and Sina، نويسنده , , R. and Swordy، نويسنده , , S.P. and Wakely، نويسنده , , S.P. and Wu، نويسنده , , J. and Yang، نويسنده , , J. and Yoon، نويسنده , , Y.S. and Zei، نويسنده , , R. and Zinn، نويسنده , , S.Y.، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2007
Pages
20
From page
1034
To page
1053
Abstract
The Cosmic Ray Energetics And Mass (CREAM) experiment is designed to investigate high-energy (1012∼1015 eV) cosmic rays over the elemental range from hydrogen to iron (1⩽Z⩽26), through a series of long balloon flights. Originally planned to be flown on the first of the new Ultra Long Duration Balloons (ULDB) being developed by NASA, the CREAM instrument was launched as a Long Duration Balloon (LDB) payload from McMurdo Station, Antarctica on December 16, 2004 and flew for a record-breaking 42 days. A second CREAM flight one year later lasted 28 days. The CREAM design is unique in that it obtains two independent energy measurements using a tungsten/scintillator sampling calorimeter and a Transition Radiation Detector (TRD) with up to four independent charge measurements of incident particles using a novel Timing-based scintillator Charge Detector (TCD), a plastic Cherenkov Detector (CD), scintillating fiber hodoscopes, and a Silicon Charge Detector (SCD). The energy limits are determined by trigger efficiency and telemetry bandwidth at the low end and by statistics at the high end.
Keywords
High-energy cosmic rays , Cosmic-ray calorimeter
Journal title
Nuclear Instruments and Methods in Physics Research Section A
Serial Year
2007
Journal title
Nuclear Instruments and Methods in Physics Research Section A
Record number
2207281
Link To Document