Particles, Plasma and Electromagnetic Waves in the Inner Heliosphere

日光层内层的粒子、等离子体和电磁波

• 批准号: 2604774
• 金额: --
• 依托单位: University of Glasgow
• 依托单位国家: 英国
• 项目类别: Studentship
• 财政年份: 2021
• 资助国家: 英国
• 起止时间: 2021 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=studentship-2604774
• 关键词: Particles; Plasma; Electromagnetic; Waves; Inner

The physics of the solar system plasma in the near-Sun environment presents a major challenge in astrophysics. This is the key region of space responsible for the birth of the solar disturbances that affects the heliosphere andforms the space weather. The new radio observations at decameter wavelength (notably with LOFAR - Low Frequency Array) will bridge the gap and will open new opportunities to study the solar phenomena in the inner heliosphere as well as the progenitors of space weather. The analysis of LOFAR radio data in combination with in-situ NASA Parker Solar Probe close to the Sun will improve our understanding of the processes in the inner heliosphere.

近太阳环境中太阳系等离子体的物理学对天体物理学提出了重大挑战。这是太空中产生影响日光层并形成太空天气的太阳扰动的关键区域。十米波长的新射电观测（特别是 LOFAR - 低频阵列）将弥补这一差距，并为研究日光层内部的太阳现象以及空间天气的起源提供新的机会。 LOFAR 无线电数据与靠近太阳的 NASA 帕克太阳探测器现场分析相结合，将增进我们对日光层内部过程的理解。