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在火星上发现极光
Jean-Loup Bertaux1, François Leblanc, Olivier Witasse
1Service d'Aéronomie du CNRS/IPSL, BP 3, Verrières-le-Buisson, 91371, France. bertaux@aerov.jussieu.fr
Nature
|June 10, 2005
概括
科学家们在火星上发现了一个独特的极光,与以前见过的不同. 这种火星极光是由地磁场异常定位和控制的,与地球和巨行星极光不同.
科学领域:
- 行星科学 行星科学
- 大气物理学 大气物理学
- 空间物理 空间物理
背景情况:
- 极光是行星大气层中由带电粒子相互作用引起的视觉辐射.
- 极光活动已知在地球,四颗巨行星和金星.
- 火星极光以前没有得到证实,金星表现出分散的,夜间排放.
研究的目的:
- 为了报告在火星大气层发现极光.
- 为了描述这个新发现的火星极光的性质.
- 为了区分火星极光与其他行星上观察到的极光.
主要方法:
- 使用了火星快速航天器上的紫外线光谱仪SPICAM.
- 分析了火星大气中的紫外线辐射.
主要成果:
- 证实了火星大气层中极光的存在.
- 确定了一种新型的极光,与地球和巨行星上的极光不同.
- 描述了火星极光高度集中和局部化.
- 确定火星极光的排放是由地磁场异常控制的.
结论:
- 火星极光代表了太阳系中新一类的极光现象.
- 与地球和巨行星不同,火星极光与极点的内在磁场线不相关.
- 火星极光的局部性质归因于行星地磁场的异常.
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