首页> 外文期刊>Space Science Reviews >A THREE-DIMENSIONAL PLASMA AND ENERGETIC PARTICLE INVESTIGATION FOR THE WIND SPACECRAFT [Review]
【24h】

A THREE-DIMENSIONAL PLASMA AND ENERGETIC PARTICLE INVESTIGATION FOR THE WIND SPACECRAFT [Review]

机译:三维空间等离子体的三维等离子体和能量粒子研究[综述]

获取原文
获取原文并翻译 | 示例
       

摘要

This instrument is designed to make measurements of the full three-dimensional distribution of suprathermal electrons and ions from solar wind plasma to low energy cosmic rays, with high sensitivity, wide dynamic range, good energy and angular resolution, and high time resolution. The primary scientific goals are to explore the suprathermal particle population between the solar wind and low energy cosmic rays, to study particle acceleration and transport and wave-particle interactions, and to monitor particle input to and output from the Earth's magnetosphere. Three arrays, each consisting of a pair of double-ended semi-conductor telescopes each with two or three closely sandwiched passivated ion implanted silicon detectors, measure electrons and ions above similar to 20 keV. One side of each telescope is covered with a thin foil which absorbs ions below 400 keV, while on the other side the incoming <400 keV electrons are swept away by a magnet so electrons and ions are cleanly separated. Higher energy electrons (up to similar to 1 MeV) and ions (up to 11 MeV) are identified by the two double-ended telescopes which have a third detector. The telescopes provide energy resolution of Delta E/E approximate to 0.3 and angular resolution of 22.5 degrees x 36 degrees, and full 4 pi steradian coverage in one spin (3 s). Top-hat symmetrical spherical section electrostatic analyzers with microchannel plate detectors are used to measure ions and electrons from similar to 3 eV to 30 keV. All these analyzers have either 180 degrees or 360 degrees fields of view in a plane, Delta E/E approximate to 0.2, and angular resolution varying from 5.6 degrees (near the ecliptic) to 22.5 degrees. Full 4 pi steradian coverage can be obtained in one-half or one spin. A large and a small geometric factor analyzer measure ions over the wide flux range from quiet-time suprathermal levels to intense solar wind fluxes. Similarly two analyzers are used to cover the wide range of electron fluxes. Moments of the electron and ion distributions are computed on board. In addition, a Fast Particle Correlator combines electron data from the high sensitivity electron analyzer with plasma wave data from the WAVE experiment (Bougeret et al., in this volume) to study wave-particle interactions on fast time scales. The large geometric factor electron analyzer has electrostatic deflectors to steer the field of view and follow the magnetic field to enhance the correlation measurements. [References: 27]
机译:该仪器旨在测量从太阳风等离子体到低能宇宙射线的超热电子和离子的完整三维分布,具有高灵敏度,宽动态范围,良好的能量和角分辨率以及高时间分辨率。主要的科学目标是探索太阳风和低能宇宙射线之间的超热粒子群,研究粒子的加速,传输和波粒相互作用,并监视粒子进入地球磁层和从地球磁层输出。三个阵列,每个由一对双端半导体望远镜组成,每个望远镜具有两个或三个紧密夹住的钝化离子注入硅探测器,可测量高于20 keV的电子和离子。每个望远镜的一侧覆盖着一层薄薄的箔片,该箔片吸收低于400 keV的离子,而在另一侧,进入的<400 keV的电子被磁铁扫走,因此电子和离子可以干净地分开。两个具有第三个探测器的双端望远镜可识别出更高能的电子(高达1 MeV)和离子(高达11 MeV)。望远镜提供的Delta E / E能量分辨率大约为0.3,角分辨率为22.5度x 36度,并在一圈(3 s)内完全覆盖了4 pi Steradian。带有微通道板检测器的高顶对称球形断面静电分析仪用于测量大约3 eV至30 keV的离子和电子。所有这些分析仪在平面上的视野均为180度或360度,Delta E / E约为0.2,角分辨率在5.6度(黄道附近)至22.5度之间变化。可以通过一半或一次旋转获得4 pi的全球面度。大型和小型几何因子分析仪可测量从安静时间超热能级到强烈的太阳风通量的宽通量范围内的离子。同样,使用两个分析仪来覆盖大范围的电子通量。电子和离子分布的矩在船上计算。另外,快速粒子相关器将来自高灵敏度电子分析仪的电子数据与来自WAVE实验的等离子体波数据结合在一起(Bougeret等人,在此体积中),以研究快速时间尺度上的波粒相互作用。大型几何因子电子分析仪具有静电偏转器,可控制视野并跟随磁场以增强相关性测量。 [参考:27]

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号