首页> 外文会议>Annual AIAA/USU conference on small satellites;AIAA/USU conference on small satellites >STEIN (SupraThermal Electrons, Ions and Neutrals), A New Particle Detection Instrument for Space Weather Research with CubeSats
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STEIN (SupraThermal Electrons, Ions and Neutrals), A New Particle Detection Instrument for Space Weather Research with CubeSats

机译:STEIN(超热电子,离子和中性粒子),一种使用CubeSat进行空间天气研究的新型粒子探测仪器

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The Space Sciences Laboratory at UC Berkeley is proposing a 3U CubeSat mission, the CubeSat for Ions, Neutrals, Electrons, and MAgnetic fields (CINEMA), to be funded by the NSF Space Weather CubeSat program and Kyung Hee University, S. Korea. CINEMA will have a particle detector called STEIN (SupraThermal Electrons, Ions, and Neutrals), part of a new breed of highly capable, low mass, and low power consumption silicon semiconductor detectors (SSDs). STEIN will measure particles in the ~2-100 keV range and distinguish between electrons, ions and neutrals up to -20 keV. It will perform fundamental research on magnetic storms and the storm-time ring current, charged particle precipitation, and electron microbursts. STEIN separates electrons, ions, and neutral atoms with an electrostatic deflection system. It has analog electronics with a very low energy threshold and a mechanical attenuator that lowers the particle count by 10~2. Using a data decimation scheme and the attenuator, STEIN can measure particle fluxes as high as 10~8 (cm~2 s sr keV)~(-1). Preliminary tests of a prototype indicate that the electrostatic deflection system works as expected. After a complete set of tests, a flight version of the instrument will be assembled, in anticipation of a possible launch in 2011.
机译:加州大学伯克利分校的太空科学实验室正在提议一项3U CubeSat任务,即用于离子,中性,电子和电磁场的CubeSat(CINEMA),由NSF太空天气CubeSat计划和韩国庆熙大学资助。 CINEMA将拥有一个名为STEIN(超热电子,离子和中性粒子)的粒子探测器,这是新一代高性能,低质量和低功耗的硅半导体探测器(SSD)的一部分。 STEIN将测量〜2-100 keV范围内的粒子,并区分电子,离子和高达-20 keV的中性粒子。它将对磁暴,暴风时环电流,带电粒子沉淀和电子微爆裂进行基础研究。 STEIN通过静电偏转系统分离电子,离子和中性原子。它具有模拟电子器件,其能量阈值非常低,并且具有机械衰减器,可将颗粒数降低10〜2。使用数据抽取方案和衰减器,STEIN可以测量高达10〜8(cm〜2 s sr keV)〜(-1)的粒子通量。原型的初步测试表明,静电偏转系统按预期工作。经过一整套测试之后,将组装该飞行器的飞行版本,以期有望在2011年推出。

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