X-ray studies of planets in our solar system

对太阳系行星的 X 射线研究

• 批准号: 2062546
• 金额: --
• 依托单位: University College London
• 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-2062546
• 关键词: ray; studies; planets; our; solar

The Chandra and XMM-Newton observatories have revealed the beauty and multiplicity of X-ray emissions from planets and comets in our solar system. The project focuses on Jupiter, with the possibility of extending to studies of our own Earth. Jupiter's polar regions show bright soft X-ray aurorae, with a line-rich spectrum arising from the charge exchange interactions of atmospheric neutrals with local and/or solar wind high charge-state heavy ions, accelerated in the planet's powerful magnetic environment. Jupiter's atmosphere also scatters solar X-rays, so that at low latitudes the planet's disk displays an X-ray spectrum that closely resembles that of solar flares. The project will make use of Chandra and XMM-Newton data to extend our current studies of the role that the solar wind plays in the X-ray aurora generation on Jupiter. Most of the data are already in hand and more will be obtained in the near future, while the JUNO spacecraft is orbiting the planet, allowing unprecedented multi-wavelength studies as well as correlated remote and in situ measurements.The process of charge exchange takes place also at Earth. Solar wind charge exchange (SWCX) X-ray emission is produced in the interaction of highly charged ions of the solar wind with neutral hydrogen in the Earth's exosphere: the emission's intensity is proportional to the ion and neutral densities, so is brightest in the dayside magnetosheath and the magnetospheric cusps. MSSL, in collaboration with other institutes in the UK, Europe, Canada, China and the European Space Agency, are developing a space mission called SMILE (www.mssl.ucl.ac.uk/SMILE) dedicated to studying this emission as a means to reach a better understanding of how the Earth's magnetosphere responds to the impact of the solar wind. Depending on progress, the student could investigate in particular the expected spectral characteristics of the SWCX X-ray emission.

钱德拉和xmm -牛顿天文台揭示了太阳系行星和彗星发出的美丽而多样的x射线。该项目的重点是木星，并有可能扩展到对我们地球的研究。木星的极地地区显示出明亮的软x射线极光，其谱线丰富，这是由大气中性物与本地和/或太阳风的高电荷态重离子的电荷交换相互作用产生的，在行星强大的磁环境中加速。木星的大气层也会散射太阳的x射线，因此在低纬度地区，木星的圆盘显示出与太阳耀斑非常相似的x射线光谱。该项目将利用钱德拉和xmm -牛顿的数据来扩展我们目前对太阳风在木星x射线极光产生中所起作用的研究。大多数数据已经到手，在不久的将来还会获得更多的数据，而朱诺号宇宙飞船正在绕地球运行，允许前所未有的多波长研究以及相关的远程和现场测量。电荷交换的过程也发生在地球上。太阳风电荷交换（SWCX） x射线发射是在太阳风的高电荷离子与地球外逸层的中性氢相互作用中产生的：发射强度与离子和中性密度成正比，因此在日侧磁鞘和磁层尖端最亮。MSSL与英国、欧洲、加拿大、中国和欧洲航天局的其他研究所合作，正在开发一项名为SMILE （www.mssl.ucl.ac.uk/SMILE）的太空任务，致力于研究这种辐射，以更好地了解地球磁层如何对太阳风的影响做出反应。根据进展情况，学生可以特别研究SWCX x射线发射的预期光谱特征。