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从磁场签名中识别了小彗星Hyakutake极长的离子尾巴
Nature
|April 15, 2000
概括
航天器的测量显示了彗星Hyakutake.
科学领域:
- 空间物理 空间物理
- 彗星科学 彗星科学
- 等离子体物理学的物理学
背景情况:
- 彗星尾巴,特别是离子 (等离子) 尾巴,在彗星气体被电离并加入太阳风时形成.
- 以前对彗星等离子体环境的现场测量仅限于非常接近彗星核 (<8,000公里).
- 太阳风是源自太阳的离子化物质的持续外流.
研究的目的:
- 报告首次在位测量彗星的等离子体尾巴,距离彗星核有很大距离.
- 描述来自太阳遥远的海库塔克彗星等离子体尾巴的结构和尺寸.
主要方法:
- 一艘航天器偶然穿过了彗星海库塔克 (C/1996 B2) 的等离子体尾部.
- 现场测量是在距离彗星核超过3.8天文单位 (55亿公里) 的距离进行的.
主要成果:
- 彗星Hyakutake的等离子尾巴被测量在3.8AU以上,远远超过以前研究的彗星.
- 测量结果证实尾巴是一个有结构的实体,直径至少为700万公里.
- 这一观测超过了1843年大三月彗星之前记录的2AU尾巴长度.
结论:
- 彗星等离子体尾巴可以是广泛的,结构化的实体,延伸数百万公里到太空.
- 远离原子核的现场测量对于了解彗星等离子体环境的全部规模和性质至关重要.
- 这些发现为彗星和太阳风之间的相互作用提供了新的见解.
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