直接探测宇宙射线:通过粒子通量精确测量的新时代

E. Mocchiutti
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引用次数: 7

摘要

在过去几年中,由于有可能在长时间的气球飞行、卫星和国际空间站上进行实验,直接测量宇宙射线的工作得到了推进。所收集的统计数据的增加和探测器结构的技术改进使通量测量能够在更高的能量下进行,并且减少了不同实验之间与过去的差异。然而,高统计精度并不总是与系统估计所需的精度相关联;粒子谱中的特征可能被错误地引入或隐藏。将对直接宇宙射线测量的最新实验结果进行审查和比较,特别强调它们的相似性和差异。
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Direct detection of cosmic rays: through a new era of precision measurements of particle fluxes

In the last years the direct measurement of cosmic rays received a push forward by the possibility of conducting experiments on board long duration balloon flights, satellites and on the International Space Station. The increase in the collected statistics and the technical improvements in the construction of the detectors permit the fluxes measurement to be performed at higher energies with a reduced discrepancy among different experiments respect to the past. However, high statistical precision is not always associated to the needed precision in the estimation of systematics; features in the particle spectra can be erroneously introduced or hidden. A review and a comparison of the latest experimental results on direct cosmic rays measurements will be presented with particular emphasis on their similarities and discrepancies.

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Contents Editorial Board Author index Hybrid Simulations of Particle Acceleration at Shocks Using optical lines to study particle acceleration at supernova remnants
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