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...

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Bibliographic Details
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
Description
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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