火星探测器大气结构调查/气象学 (ASI/MET) 实验
J T Schofield1, J R Barnes, D Crisp
1J. T. Schofield and D. Crisp, Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
概括
火星的路径探测器火星路径探测器
科学领域:
- 行星科学 行星科学
- 大气科学 大气科学
- 火星气象学 火星气象学
背景情况:
- 火星路径探测器任务提供了有关火星大气条件的宝贵数据.
- 之前的任务,如维京1着陆器 (VL-1) 建立了火星天气的基准.
- 了解火星大气对于未来的探索和可居住性研究至关重要.
研究的目的:
- 测量火星大气层的垂直结构 (密度,压力,温度) 到160公里.
- 为了监测火星83个月的地表气象和气候.
- 为了将当前的火星大气数据与维京1登陆器的历史记录进行比较.
主要方法:
- 在火星路径探测器着陆器上利用大气结构调查/气象学 (ASI/MET) 实验.
- 收集大气密度,压力和温度概况的数据.
- 监测表面天气现象,包括风,温度和压力变化.
主要成果:
- 大气结构和天气模式与维京1号着陆器的观测结果相似.
- 观察到的差异包括更冷的夜间上层大气层和更温暖的表面温度 (10-12 K增加).
- 通过其独特的压力,风和温度签名来识别倾斜控制的风和尘埃魔.
结论:
- 火星大气层与温暖,中度灰尘的环境是一致的,正如之前VL-1所建议的那样.
- 昼间的影响和着陆地点的表面特性影响大气条件.
- 火星探测器的数据提升了我们对火星大气动态和气候的理解.
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