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High energy neutral atom (HENA) imager for the IMAGE mission [Review]

机译:用于IMAGE任务的高能中性原子(HENA)成像仪[评论]

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摘要

The IMAGE mission will be the first of its kind, designed to comprehensively image a variety of emissions from the Earth's magnetosphere, with sufficient time resolution to follow the dynamics associated with the development of magnetospheric storms. Energetic neutral atoms (ENA) emitted from the ring current during storms are one of the key emissions that will be imaged. This paper describes the characteristics of the High Energy Neutral Atom imager, HENA. Using pixelated solid state detectors, imaging microchannel plates, electron optics, and time of flight electronics, HENA is designed to return images of the ENA emitting regions of the inner magnetosphere with 2 minute time resolution, at angular resolution of 8 degrees or better above the energy of similar to 50 keVucleon. HENA will also image separately the emissions in hydrogen, helium, and oxygen above 30 keVucleon. HENA will reject energetic ions below 200 keV/charge, allowing ENA images to be returned in the presence of ambient energetic ions. HENA images will reveal the distribution and the evolution of energetic ion distributions as they are injected into the ring current during geomagnetic storms, as they drift about the Earth on both open and closed drift paths, and as they decay through charge exchange to pre-storm levels. Substorm ion injections will also be imaged, as will the regions of low altitude, high latitude ion precipitation into the upper atmosphere. [References: 32]
机译:IMAGE任务将是同类任务中的第一个任务,旨在对地球磁层的各种排放物进行全面成像,并具有足够的时间分辨率以跟踪与磁层风暴发展相关的动态。在暴风雨期间,环流发出的高能中性原子(ENA)是将被成像的关键发射之一。本文介绍了高能中性原子成像仪HENA的特性。通过使用像素化的固态检测器,成像微通道板,电子光学器件和飞行时间电子设备,HENA被设计为以2分钟的时间分辨率返回内部磁层ENA发射区域的图像,其角分辨率为8度或更高。能量类似于50 keV /核仁。 HENA还将分别对30 keV /核仁以上的氢,氦和氧的排放进行成像。 HENA将拒绝低于200 keV /电荷的高能离子,从而在存在环境高能离子的情况下返回ENA图像。 HENA图像将揭示在地磁暴期间注入环流中的高能离子分布的分布和演变,它们在开放和闭合漂移路径上绕地球漂移以及通过电荷交换衰减到暴风前的过程水平。亚暴离子注入也将被成像,低海拔,高纬度离子沉淀到高层大气的区域也将被成像。 [参考:32]

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