Nuclear Instruments and Methods in Physics r Ah J.T
10 to 10 eV and abundance changes that might be related to the supernova acceleration limit [1]. three orbits around the South Pole. The CREAM employs a suite of particle detectors to determine the charge and energy of cosmic rays. Energy is ARTICLE IN PRESSmeasured by two independent detectors: a s...
Main Authors: | , , , , , , , , , |
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Language: | English |
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Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.503.6091 http://cosmicray.umd.edu/cream/images/stories/files/frontpage/SCD_NIMA_570_2007_286_291.pdf |
Summary: | 10 to 10 eV and abundance changes that might be related to the supernova acceleration limit [1]. three orbits around the South Pole. The CREAM employs a suite of particle detectors to determine the charge and energy of cosmic rays. Energy is ARTICLE IN PRESSmeasured by two independent detectors: a sampling tungsten/scintillator calorimeter and a transition radiation detector with a Cherenkov Detector (CD). Both detectors 0168-9002/ $- see front matter r 2006 Elsevier B.V. All rights reserved. doi:10.1016/j.nima.2006.09.056 Corresponding author. |
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