Nuclear Instruments and Methods in Physics r Ah J.T

• Main Authors: Makingj. H. Park, E. S. Seo, R. Sina, S. Swordy, S. Wakely, J. Wu, J. Yang, Y. S. Yoon, R. Zeid, S. Y. Zinnb
• Other Authors: The Pennsylvania State University CiteSeerX Archives
• Format: Text
• Language: English
• Subjects: High-energy cosmic ray; PIN diode silicon sensor; Silicon charge detector; Balloon payload 1. Overview of the CREAM experiment; South Pole; South pole
• 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

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.