火星上层大气中的夜光以及对大气运输的影响
Jean-Loup Bertaux1, François Leblanc, Séverine Perrier
1Service d'Aéronomie du CNRS/Institut Pierre-Simon Laplace (IPSL), BP.3, 91371, Verrières-le-Buisson, France. bertaux@aerov.jussieu.fr
概括
火星快递在火星夜间大气中检测到紫外线辐射. 这种夜光,主要是氧化 (NO) 波段,在冬季的南极地区是最明亮的,这是由于大气运输和结.
科学领域:
- 行星科学 行星科学
- 大气科学 大气科学
- 频谱学是一种光谱学.
背景情况:
- 火星大气表现出复杂的化学过程,包括由太阳辐射驱动的化学过程.
- 了解大气排放对于描述行星环境至关重要.
研究的目的:
- 为了检测和分析夜间火星大气中的光辐射.
- 为了确定这些大气排放的组成和来源.
主要方法:
- 在火星快速航天器上使用了SPICAM (用于研究火星大气层特征的光谱学) 紫外线光谱仪.
- 分析了火星夜光的紫外线光谱.
主要成果:
- 在火星夜间大气中检测到气莱曼α排放和氧化 (NO) 玛和三角波段.
- NO排放的结果是 (N) 和氧 (O) 原子的重组,通过极端紫外线光解离产生.
- 在冬季的南极夜间,NO排放强度最大.
结论:
- 观测到的夜光主要由来自白天大气光解离和随后的运输的NO排放组成.
- 冬季南极夜间氧化物排放量增加的原因是不断下降的空中运输和地面结.
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