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Echo Particle Image Velocimetry
Published on: December 27, 2012
金星的动态上层大气层,由VIRTIS在Venus Express上揭示出来
P Drossart1, G Piccioni, J C Gérard
1LESIA, Observatoire de Paris, CNRS, UPMC, Université Paris-Diderot, 5 place Jules Janssen, 92195 Meudon, France. pierre.drossart@obspm.fr
Nature
|November 30, 2007
概括
测量显示,金星上层大气层 (90-120公里) 有明显的CO2和O2排放峰值. 这些数据有助于理解大气的能量和循环,特别是与氧原子运输相关的O2排放.
科学领域:
- 行星科学 行星科学
- 大气物理学 大气物理学
- 航空学是航空学的.
背景情况:
- 金星的上层大气层充当行星内部与太空之间的关键能量转移区域.
- 以前的研究表明,光化学和动态过程控制金星上层大气结构,但辐射高度仍然不清楚.
研究的目的:
- 通过分子排放来研究金星上层大气 (90-120公里) 的能量和循环.
- 精确确定金星上层大气中二氧化碳 (CO2) 和氧气 (O2) 排放的高度.
主要方法:
- 在4.3微米 (90-120公里高度) 测量日间二氧化碳非局部热力学平衡排放.
- 测量了夜间的O2排放 (95-100公里高度).
主要成果:
- 峰值二氧化碳排放量在115公里左右被观察到,显示出与太阳顶峰角度的变化.
- 峰值O2排放发生在96公里±1公里处.
- O2排放高度与通过全球热层循环预测的氧原子运输相一致.
结论:
- 这项研究证实了先前对金星上层大气中二氧化碳排放变化的建模.
- 氧气排放高度支持了亚太到反太阳循环运输氧气原子的假设.
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