AI 中文总结
本综述利用多航天器多点多仪器观测，结合Solar Orbiter与Parker Solar Probe的近太阳高能粒子测量，研究行星际日冕物质抛射和激波对高能粒子加速与传输的作用，以解决相关未决问题。
AI 中文摘要
从超热（数千电子伏特）到相对论性（数千吉电子伏特）能量的太阳高能粒子，是表征空间环境的重要组成部分。它们从太阳发射，与太阳耀斑及日冕物质抛射驱动的激波相关。本综述利用日球层中多艘航天器组成的舰队提供的多点、多仪器观测，呈现了行星际日冕物质抛射（ICME）与激波在高能粒子加速和传输研究中的重要最新成果。特别是，Solar Orbiter（太阳轨道器）和Parker Solar Probe（帕克太阳探测器）这两项开创性任务，提供了近太阳环境中高能粒子的前所未有的测量结果，为解决多个未解决问题提供了有前景的见解，这些问题尤其涉及日球层中高能粒子加速与传输的机制及其相对贡献。
英文摘要
Solar Energetic Particles from suprathermal (few keV) up to relativistic (few GeV) energies constitute an important contributor to the characterization of the space environment. Emitted from the Sun they are associated with solar flares and shock waves driven by Coronal Mass Ejections. This review presents important recent results of the study of Interplanetary CMEs and shocks in relation to energetic particle acceleration and transport, taking advantage of multi-point, multi-instrument observations available by a fleet of spacecraft in the heliosphere. In particular, the Solar Orbiter and Parker Solar Probe pioneering missions providing unprecedented measurements of energetic particles in the near-Sun environment offer promising insights into several unresolved questions particularly regarding the mechanisms responsible for the acceleration and transport of energetic particles in the heliosphere and their relative contributions.
