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Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus

机译:太阳风电子阿尔法和质子(sWEap)调查:用于太阳能探测器的太阳风和日冕等离子体仪器套件的设计

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摘要

The Solar Wind Electrons Alphas and Protons (SWEAP) Investigation on Solar Probe Plus is a four sensor instrument suite that provides complete measurements of the electrons and ionized helium and hydrogen that constitute the bulk of solar wind and coronal plasma. SWEAP consists of the Solar Probe Cup (SPC) and the Solar Probe Analyzers (SPAN). SPC is a Faraday Cup that looks directly at the Sun and measures ion and electron fluxes and flow angles as a function of energy. SPAN consists of an ion and electron electrostatic analyzer (ESA) on the ram side of SPP (SPAN-A) and an electron ESA on the anti-ram side (SPAN-B). The SPAN-A ion ESA has a time of flight section that enables it to sort particles by their mass/charge ratio, permitting differentiation of ion species. SPAN-A and -B are rotated relative to one another so their broad fields of view combine like the seams on a baseball to view the entire sky except for the region obscured by the heat shield and covered by SPC. Observations by SPC and SPAN produce the combined field of view and measurement capabilities required to fulfill the science objectives of SWEAP and Solar Probe Plus. SWEAP measurements, in concert with magnetic and electric fields, energetic particles, and white light contextual imaging will enable discovery and understanding of solar wind acceleration and formation, coronal and solar wind heating, and particle acceleration in the inner heliosphere of the solar system. SPC and SPAN are managed by the SWEAP Electronics Module (SWEM), which distributes power, formats onboard data products, and serves as a single electrical interface to the spacecraft. SWEAP data products include ion and electron velocity distribution functions with high energy and angular resolution. Full resolution data are stored within the SWEM, enabling high resolution observations of structures such as shocks, reconnection events, and other transient structures to be selected for download after the fact. This paper describes the implementation of the SWEAP Investigation, the driving requirements for the suite, expected performance of the instruments, and planned data products, as of mission preliminary design review.
机译:Solar Probe Plus上的太阳风电子质子(SWEAP)研究是一套四传感器仪器套件,可对构成太阳风和日冕等离子体的大部分电子,离子化的氦和氢进行完整的测量。 SWEAP由太阳探针杯(SPC)和太阳探针分析仪(SPAN)组成。 SPC是一个法拉第杯,直接看向太阳,并测量离子和电子通量以及流动角与能量的关系。 SPAN由位于SPP冲压侧(SPAN-A)的离子和电子静电分析仪(ESA)和位于反冲压侧(SPAN-B)的电子ESA组成。 SPAN-A离子ESA具有飞行时间截面,可使其按质荷比对颗粒进行分类,从而区分离子种类。 SPAN-A和-B彼此相对旋转,因此它们的宽视野像棒球上的接缝一样结合在一起,可以看到整个天空,除了被隔热罩遮盖并被SPC覆盖的区域。 SPC和SPAN的观测产生了满足SWEAP和Solar Probe Plus科学目标所需的综合视场和测量能力。 SWEAP测量与磁场,电场,高能粒子和白光上下文成像相结合,将使人们能够发现和理解太阳风的加速和形成,日冕和太阳风的加热以及太阳系内部太阳圈中的粒子加速。 SPC和SPAN由SWEAP电子模块(SWEM)进行管理,该模块可以分配电源,格式化机载数据产品,并充当与航天器的单个电气接口。 SWEAP数据产品包括具有高能量和角分辨率的离子和电子速度分布函数。全分辨率数据存储在SWEM内,从而可以对诸如冲击,重新连接事件和其他瞬态结构之类的结构进行高分辨率观察,然后再进行下载。本文描述了SWEAP调查的实施情况,套件的驾驶要求,仪器的预期性能以及计划的数据产品,以及特派团的初步设计审查。

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