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arXiv 1003.4983astro-ph.HEastro-ph.IM
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CREAM-I飞行的元素光谱

Elemental Spectra from the CREAM-I Flight

H. S. Ahn, P. Allison, M. G. Bagliesi, J. J. Beatty, G. Bigongiari, P. Boyle, J. T. Childers, N. B. Conklin, S. Coutu, M. A. Duvernois, O. Ganel, J. H. Han, J. … 展开作者

H. S. Ahn, P. Allison, M. G. Bagliesi, J. J. Beatty, G. Bigongiari, P. Boyle, J. T. Childers, N. B. Conklin, S. Coutu, M. A. Duvernois, O. Ganel, J. H. Han, J. A. Jeon, K. C. Kim, J. K. Lee, M. H. Lee, L. Lutz, P. Maestro, A. Malinine, P. S. Marrocchesi, S. Minnick, S. I. Mognet, S. Nam, S. Nutter, I. H. Park, N. H. Park, E. S. Seo, R. Sina, S. Swordy, S. Wakely, J. Wu, J. Yang, Y. S. Yoon, R. Zei, S. Y. Zinn

摘要:

宇宙射线能量学和质量(CREAM)是一个气球实验,旨在测量电荷Z = 1至26的宇宙射线的成分和能谱,能量高达~ 10^15 eV。2004年12月和2005年12月,CREAM利用从南极洲Mc Murdo站发射的长时间气球进行了两次成功的飞行。CREAM-I通过采用多个探测器系统实现了大量的测量冗余,即用于粒子识别的定时电荷探测器和硅电荷探测器(SCD),以及用于能量测量的过渡辐射探测器和采样钨/闪烁纤维电离量热计(CAL)。本文介绍了在第一个42天的飞行期间,用CAL/SCD测量的各种元素的初步能谱。

英文摘要:

The Cosmic Ray Energetics And Mass (CREAM) is a balloon-borne experiment designed to measure the composition and energy spectra of cosmic rays of charge Z = 1 to 26 up to an energy of ~ 10^15 eV. CREAM had two successful flights on long-duration balloons (LDB) launched from Mc- Murdo Station, Antarctica, in December 2004 and December 2005. CREAM-I achieves a substantial measurement redundancy by employing multiple detector systems, namely a Timing Charge Detector and a Silicon Charge Detector (SCD) for particle identification, and a Transition Radiation Detector and a sampling tungsten/scintillating-fiber ionization calorimeter (CAL) for energy measurement. In this paper, preliminary energy spectra of various elements measured with CAL/SCD during the first 42-day flight are presented.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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