Magnetosphere-Ionosphere Coupling at the Outer Planets

外行星的磁层-电离层耦合

• 批准号: 2107533
• 金额: --
• 依托单位: University of Leicester
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2018
• 资助国家: 英国
• 起止时间: 2018 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2107533
• 关键词: Magnetosphere; Ionosphere; Coupling; Outer; Planets

Since 2016, for the first time in space history, there have been two outer planet missions operating at Jupiter (NASA Juno) and Saturn (NASA-ESA Cassini) simultaneously. The end-of-Cassini mission sequence took place on Sept 15th 2017, after the Grand Finale orbits where the spacecraft plummeted between the inner edge of the ring system and Saturn itself. From a data gathering perspective, this dramatic end of mission sequence has taken us into completely unexplored regions of the Saturn system, and we have gathered much new data from this final episode of the mission. This adds to the previous 12 years of continuous operations at Saturn, yielding a 13 year dataset which is yet to be fully exploited scientifically.The Juno mission entered orbit at Jupiter in July 2016. The spacecraft is now in a 53 day orbit, exploring the polar regions of Jupiter's magnetosphere, providing unprecedented data from the various instruments on board. Each periapsis pass (every 53 days) provides a wealth of new information on the coupling between the magnetosphere and the ionosphere, and the dynamics of the planet's auroral emissions in the upper atmosphere.Both missions have been supported by Leicester-led Hubble Space Telescope campaigns to study the ultra-violet auroras to complement and extend the UV/IR observations taken by both spacecraft from Jupiter and Saturn orbit.We are the only UK group involved in the Juno mission (as Science CoIs) and have access to data during the proprietary period, e.g. we have full access to the energetic particle data from the JEDI instrument.We have been involved in the Cassini mission since the beginning, and are CoIs on the magnetometer team and thus have a great deal of experience of working with this data set and others (e.g. plasma, radio and plasma waves, UV/IR).In this PhD project, there will be scope to work on either the Cassini mission data and/or the Juno mission data. The student will be studying aspects of solar wind-magnetosphere-ionosphere coupling at either/both planet, including data analysis of in situ spacecraft datasets and remote sensing data from the Hubble Space Telescope.

自2016年以来，在太空历史上第一次有两个外行星任务同时在木星（NASA朱诺号）和土星（NASA-ESA卡西尼号）运行。卡西尼号使命序列的结束发生在2017年9月15日，在大结局轨道之后，航天器在环系统的内边缘和土星本身之间暴跌。从数据收集的角度来看，这一戏剧性的使命序列的结束将我们带到了土星系统中完全未被探索的区域，我们从使命的最后一集收集了许多新的数据。这增加了之前12年在土星的连续运行，产生了13年的数据集，尚未被充分科学利用。朱诺号使命于2016年7月进入木星轨道。该航天器目前在53天的轨道上，探索木星磁层的极地地区，从船上的各种仪器提供前所未有的数据。每次近心点通过（每53天）提供了大量关于磁层和电离层之间耦合的新信息，以及地球高层大气中极光发射的动力学。这两项任务都得到了莱斯特领导的哈勃太空望远镜活动的支持，以研究紫外极光，补充和扩展紫外/两个航天器从木星和土星轨道进行的红外观测。我们是唯一参与朱诺使命的英国小组（作为科学委员会），并在专有期间访问数据，例如，我们完全可以使用JEDI仪器的高能粒子数据。我们从一开始就参与了卡西尼号的使命，是磁强计团队的CoI，因此在使用此数据集和其他数据集方面具有丰富的经验（例如等离子体、无线电和等离子体波、紫外线/红外线）。在这个博士项目中，将有范围研究卡西尼号使命数据和/或朱诺号使命数据。该学生将研究太阳风磁层电离层耦合在任一/两个行星的方面，包括现场航天器数据集和哈勃太空望远镜遥感数据的数据分析。