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首页> 外文期刊>Space Science Reviews >Electron, Proton, and Alpha Monitor on the advanced composition explorer spacecraft [Review]
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Electron, Proton, and Alpha Monitor on the advanced composition explorer spacecraft [Review]

机译:先进的成分探测器太空船上的电子,质子和Alpha监视器[评论]

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摘要

The Electron, Proton, and Alpha Monitor (EPAM) is designed to make measurements of ions and electrons over a broad range of energy and intensity. Through five separate solid-state detector telescopes oriented so as to provide nearly full coverage of the unit-sphere, EPAM can uniquely distinguish ions (E(i)greater than or similar to 50 keV) and electrons (E(e)greater than or similar to 40 keV) providing the context for the measurements of the high sensitivity instruments on ACE. Using a Delta E x E telescope, the instrument can determine ion elemental abundances (E greater than or similar to 0.5 MeV nucl(-1)). The large angular coverage and high time resolution will serve to alert the other instruments on ACE of interesting anisotropic events. The experiment is controlled by a microprocessor-based data system, and the entire instrument has been reconfigured from the HI-SCALE instrument on the Ulysses spacecraft. Inflight calibration is achieved using a variety of radioactive sources mounted on the reclosable telescope covers. Besides the coarse (8 channel) ion and (4 channel) electron energy spectra, the instrument is also capable of providing energy spectra with 32 logarithmically spaced channels using a pulse-height-analyzer. The instrument, along with its mounting bracket and radiators weighs 11.8 kg and uses about 4.0 W of power. To demonstrate some of the capabilities of the instrument, some initial performance data are included from a solar energetic particle event in November 1997. [References: 5]
机译:电子,质子和Alpha监测器(EPAM)旨在测量各种能量和强度范围内的离子和电子。通过定向的五个独立的固态探测器望远镜可以几乎完全覆盖单位球面,EPAM可以唯一地区分离子(E(i)大于或类似于50 keV)和电子(E(e)大于或大于50 keV)。类似于40 keV)为ACE上的高灵敏度仪器的测量提供了环境。使用Delta E x E望远镜,仪器可以确定离子元素丰度(E大于或类似于0.5 MeV nucl(-1))。大的角度覆盖范围和较高的时间分辨率将有助于提醒ACE上的其他仪器注意有趣的各向异性事件。该实验由基于微处理器的数据系统控制,并且整个仪器已经从Ulysses航天器上的HI-SCALE仪器进行了重新配置。使用安装在可重新闭合的望远镜盖上的各种放射源可以实现机内校准。除了粗略的(8通道)离子和(4通道)电子能谱外,该仪器还能够使用脉冲高度分析仪提供32个对数间隔的通道的能谱。该仪器及其安装支架和散热器重11.8千克,使用约4.0瓦功率。为了演示该仪器的某些功能,在1997年11月的一次太阳高能粒子事件中包含了一些初始性能数据。[参考文献:5]

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