A Comparative Study of Metallic Ions in the Atmospheres of Earth and Mars

地球和火星大气中金属离子的比较研究

• 批准号: 2481388
• 金额: --
• 依托单位: University of Leeds
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2020
• 资助国家: 英国
• 起止时间: 2020 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2481388
• 关键词: Comparative; Study; Metallic; Ions; Atmospheres

Metals are injected into planetary atmospheres by the ablation of interplanetary dust particles. The major species (Fe, Mg and Na) exist as atoms and ions that are excellent tracers of dynamics and chemistry. This project will contrast the behaviour of these metals in the Martian and terrestrial atmospheres. On Earth, metals are observed by ground-based lidar, rocket-borne mass spectrometry, and from optical spectrometers on satellites. For Mars, NASA's MAVEN spacecraft is providing unprecedented measurements of metallic ions over much of the planet's ionosphere. This is because MAVEN's highly elliptical orbit permits sampling to unusually low altitudes. Surprisingly different behaviour in the metal ions has been observed, which is probably due to (at least) two factors: unlike the Earth which has a permanent magnetic field, Mars only has patches of crustal magnetism mainly in the southern hemisphere; and Mars has a CO2 - rather than an N2/O2 - atmosphere.This project will used global whole-atmosphere models of Earth and Mars to understand why the metals behave so differently. The objective will be to improve our understanding of the coupling between the neutral and ionized atmosphere. An important reason for doing so is to understand the effects of space weather on our atmosphere, both short-term perturbations and longer-term climatic influences. The two models that will be employed are WACCM-X, an extended version of the Whole Atmosphere Community Climate Model from the National Center for Atmospheric Research (Boulder, USA), and the LMD-Mars model from the CNRS in Paris. Both are available at Leeds. This project will provide a high level of specialist scientific training in: (i) the application of world-leading atmospheric chemistry-climate models; (ii) analysis and synthesis or large datasets; (iii) use of advanced High Performance Computing facilities.

金属是通过行星际尘埃粒子的烧蚀而注入行星大气层的。主要物种（Fe、Mg和Na）以原子和离子的形式存在，它们是动力学和化学的优良示踪剂。该项目将对比这些金属在火星和地球大气中的行为。在地球上，金属是通过地面激光雷达、火箭载质谱仪和卫星上的光学光谱仪观测到的。对于火星，美国宇航局的MAVEN航天器正在提供前所未有的测量金属离子在大部分行星的电离层。这是因为MAVEN的高度椭圆轨道允许在异常低的高度进行采样。已经观察到金属离子中令人惊讶的不同行为，这可能是由于（至少）两个因素：不像地球有永久磁场，火星只有主要在南半球的地壳磁场;火星的大气层是二氧化碳，而不是氮气和氧气。这个项目将使用全球的整体-地球和火星的大气模型，以了解为什么金属的行为如此不同。其目的是提高我们对中性和电离大气之间的耦合的理解。这样做的一个重要原因是了解空间天气对我们大气层的影响，包括短期扰动和长期气候影响。将采用的两个模型是WACCM-X，这是美国国家大气研究中心（博尔德）的全大气社区气候模型的扩展版本，以及巴黎的CNRS的LMD-Mars模型。这两种都在利兹有售。该项目将在以下方面提供高水平的专业科学培训：（一）世界领先的大气化学-气候模型的应用;（二）大型数据集的分析和综合;（三）先进的高性能计算设施的使用。