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A FARADAY-CUP SOLAR WIND EXPERIMENT FOR SOLAR ORBITER

机译:太阳能轨道飞行杯太阳能实验

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We propose a design for a Faraday Cup instrument that could perform rapid measurements of solar wind hydrogen and helium on Solar Orbiter. Considering the instrument requirements described in the straw man payload, a Faraday Cup has many virtues in comparison with other instrument designs. First, the Faraday Cup is not sensitive to contamination. Second, the detector (a metal collector plate) is insensitive to radiation and photons. This will be a very significant factor for Solar Orbiter. Experience with the Faraday Cup system onboard the Wind spacecraft has shown a drift in the absolute response of the instrument of less than 0.1% per decade. That stability is ideal for an instrument on a spacecraft operating alone in a harsh environment. Third, the Faraday Cup would have a wide-angular acceptance (45° half-angle cone). This would enable accurate measurements of Alfven wave fluctuations. Finally, the Faraday Cup has a demonstrated track record of accurate measurements of ion beams and temperature anisotropies that have led to new scientific understanding of the instabilities that will be a key part of Solar Orbiter. We propose a Faraday Cup that would make rapid, 10-Hz measurements of three-dimensional properties of solar wind hydrogen and helium: velocities, temperatures, heat fluxes, beams, and anisotropies. A subset of these data would be sent to Earth, but the high time resolution measurements would be correlated on board with measurements of the local electric field, leading to a new understanding of the physics of dissipation and heating in the solar wind.
机译:我们提出了一个关于法拉第杯仪器的设计,可以在太阳能轨道上进行太阳能氢气和氦的快速测量。考虑到秸秆人有效载中描述的仪器要求,与其他乐器设计相比,法拉第杯具有许多优点。首先,法拉第杯对污染不敏感。其次,检测器(金属收集板)对辐射和光子不敏感。这将是太阳能轨道运动员的一个非常重要的因素。在风宇宙飞车上使用法拉第杯系统的经验表明,仪器绝对响应的漂移量小于每十年的0.1%。这种稳定性非常适用于在恶劣环境中单独操作的航天器上的乐器的理想选择。第三,法拉第杯将具有宽角度验收(45°半角锥)。这将能够准确测量Alfven波波波动。最后,法拉第杯具有用于离子束和温度各向异性的准确测量的轨道记录,这些是对太阳能轨道飞机的关键部分的新的科学了解。我们提出了一杯法拉第杯,该杯将使太阳风氢气和氦气的三维特性进行快速,10 Hz测量:速度,温度,热助熔剂,梁和各向异性。这些数据的子集将被发送到地球,但是高时间分辨率测量将在船上与局部电场的测量相关,导致对太阳风中的耗散和加热的物理学的新了解。

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