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首页> 外文期刊>Physical review letters >Electron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station
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Electron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station

机译:在国际空间站上使用阿尔法磁谱仪测量的主要宇宙射线中的电子和正电子通量

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摘要

Precision measurements by the Alpha Magnetic Spectrometer on the International Space Station of the primary cosmic-ray electron flux in the range 0.5 to 700 GeV and the positron flux in the range 0.5 to 500 GeV are presented. The electron flux and the positron flux each require a description beyond a single power-law spectrum. Both the electron flux and the positron flux change their behavior at ~30 GeV but the fluxes are significantly different in their magnitude and energy dependence. Between 20 and 200 GeV the positron spectral index is significantly harder than the electron spectral index. The determination of the differing behavior of the spectral indices versus energy is a new observation and provides important information on the origins of cosmic-ray electrons and positrons.
机译:介绍了国际空间站上的Alpha电磁光谱仪对0.5至700 GeV范围内的主要宇宙射线电子通量和0.5至500 GeV范围内的正电子通量的精确测量。电子通量和正电子通量都需要超出单个幂律谱的描述。电子通量和正电子通量都在〜30 GeV时改变其行为,但通量在大小和能量依赖性方面存在显着差异。在20 GeV和200 GeV之间,正电子光谱指数明显比电子光谱指数硬。光谱指数与能量的不同行为的确定是一个新发现,它提供了有关宇宙射线电子和正电子起源的重要信息。

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