针对IMAP任务的紧型双离子组成实验 (CoDICE)
S A Livi1,2, M I Desai1,2, K Ogasawara1,2
1Space Science & Engineering, Southwest Research Institute, San Antonio, USA.
概括
美国宇航局的IMAP任务使用CoDICE仪器研究太阳风和星际相互作用. 它测量带电粒子,并为太空天气研究提供对当地的星际介质的见解.
科学领域:
- 太空物理学 太空物理学
- 空间物理 空间物理
- 等离子体物理学的物理学
背景情况:
- 太阳-地球拉格朗日点L1是观测太阳风和星际介质相互作用的战略位置.
- 了解日球界限对于太空天气预测和基本等离子体物理学至关重要.
研究的目的:
- 详细介绍了NASA的IMAP任务上的紧型双离子组成实验 (CoDICE) 仪器.
- 分析带电粒子加速和太阳风与当地的星际介质的相互作用.
- 用星际拾取离子研究当地的星际介质的特性.
主要方法:
- CoDICE采用了一种新的,紧的设计,结合了两个测量系统.
- 它测量了3D速度分布函数和低能粒子 (0.5-80 keV/q) 的组成.
- 它确定了高能离子 (0.03-5 MeV/nuc) 的到达方向和组成.
主要成果:
- CoDICE提供了太阳风,超热和拾取离子的全面测量.
- 它描述了星际He+离子和He和Ne拾取离子的同位素组成.
- 太阳风丰度,电荷状态和质子强度的实时数据可用于太空天气监测.
结论:
- CoDICE是一款下一代仪器,可对当地的星际介质和日球进行详细研究.
- 它的测量有助于理解带电粒子加速和太阳风-日球相互作用.
- 该仪器支持基础空间物理研究和操作空间天气监测.
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