Laboratory Studies of O2 Excited States Relevant to the CO2 Planets

与 CO2 行星相关的 O2 激发态的实验室研究

• 批准号: 1109372
• 负责人: Konstantinos Kalogerakis
• 金额: $ 33.99万
• 依托单位: SRI International
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2011
• 资助国家: 美国
• 起止时间: 2011-09-01 至 2014-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1109372&HistoricalAwards=false
• 关键词: Laboratory; Studies; O2; Excited; States

In the upper atmospheres of Venus, Earth, and Mars, molecular oxygen is dissociated into atomic oxygen by absorption of solar ultraviolet radiation. The oxygen atoms can then recombine through a 3-body interaction with another molecule to form molecular oxygen in an excited state. On Venus and Mars, the third molecule is carbon dioxide. The competition between photodissociation, recombination, and diffusive transport determines the atomic and molecular composition of the mesosphere and lower thermosphere. Accurate knowledge of the oxygen atom recombination processes is critical for modeling the diurnal behavior of the altitude profile of oxygen atoms and interpreting nightglow emissions from atomic oxygen, molecular oxygen, and hydroxyl. In this project, the Principal Investigator and a postdoctoral fellow will conduct laboratory experiments to study the yields of the excited molecular oxygen states generated following O-atom recombination in a carbon dioxide environment. An ultraviolet light pulse from an excimer laser will photoinitiate O-atom recombination in carbon dioxide, maintained in a temperature-controlled gas flow cell. Fluorescence and resonance enhanced multiphoton ionization (REMPI) techniques will detect excited oxygen molecules and determine the yields of the excited states produced following O-atom recombination and subsequent relaxation in carbon dioxide. These measurements are needed to quantify oxygen airglow in the upper atmospheres of Venus and Mars and to probe their atmospheric dynamics by remote sensing. The results will benefit modelers of planetary atmospheres and will enhance the scientific returns on past and future missions to Venus and Mars. Application of basic chemistry and physics to the study of collisional processes is also critical for understanding the operation of high-power chemical lasers. Finally, the project will contribute to the training and research experience of a postdoctoral fellow and summer undergraduate students.

在金星、地球和火星的高层大气中，分子氧被太阳紫外线辐射吸收解离为原子氧。然后，氧原子可以通过与另一个分子的三体相互作用重新结合，形成处于激发态的分子氧。在金星和火星上，第三种分子是二氧化碳。光解离、复合和扩散输运之间的竞争决定了中间层和低热层的原子和分子组成。对氧原子复合过程的准确了解对于模拟氧原子高度分布的日行为和解释原子氧、分子氧和羟基的夜辉发射是至关重要的。在这个项目中，首席研究员和一名博士后研究员将进行实验室实验，研究二氧化碳环境中氧原子复合产生的激发分子氧态的产率。来自准分子激光的紫外光脉冲将在二氧化碳中光引发O原子复合，保持在温度控制的气体流动池中。荧光和共振增强多光子电离(REMPI)技术将检测被激发的氧分子，并确定在二氧化碳中氧原子复合和随后的弛豫所产生的激发态的产率。需要这些测量来量化金星和火星上层大气中的氧气气辉，并通过遥感探测它们的大气动力学。这一结果将有利于行星大气的建模人员，并将提高过去和未来前往金星和火星任务的科学回报。将基础化学和物理学应用于碰撞过程的研究，对于理解高功率化学激光器的运行也是至关重要的。最后，该项目将有助于博士后研究员和暑期本科生的培训和研究经验。