首页> 外文会议>Space Technology amp; Applications International Forum (STAIF-99) ptol January 31-February 4, 1999, Albuquerque Hyatt Hotel, NM >Ultra heavy (Z>30) and heavy (10<=Z<=30) cosmic-ray measurements on ACCESS with the charge (Z) identification module (ZIM)
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Ultra heavy (Z>30) and heavy (10<=Z<=30) cosmic-ray measurements on ACCESS with the charge (Z) identification module (ZIM)

机译:使用电荷(Z)识别模块(ZIM)在ACCESS上进行超重(Z> 30)和重(10 <= Z <= 30)宇宙射线测量

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The Charge (Z) identification Module (ZIM) for ACCESS has as its primary objective the measurement of the cosmic-ray abundance of every individual element in the interval 10<=Z<=83 with cleanly resolved individual element resolution and with sufficient collection power to give exceelent statistical significance. This instrument will, for the first time, determine the full element-by-element composition of cosmic rays, througout the heavy two-thirds of the periodic table, providing definitive tests of theories of sites and mechanisms of cosmic-ray acceleration. We expect that detectors with this UH configuration will srve as the Charge Module for the full ACCESS instrument. In this paper we describe the science objectives of ZIM and the measurements that can be achieved with this instrument.
机译:用于ACCESS的电荷(Z)识别模块(ZIM)的主要目标是,以清晰分辨的单个元素分辨率和足够的采集能力,测量10 <= Z <= 83区间中每个单个元素的宇宙射线丰度具有卓越的统计意义。该仪器将首次确定整个宇宙射线的各个元素的完整组成,排除了三分之二的重原子周期,为宇宙射线加速的场所理论和机理提供了确定的检验。我们希望具有这种UH配置的检测器将成为整个ACCESS仪器的充电模块。在本文中,我们描述了ZIM的科学目标以及该仪器可以实现的测量。

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