Flaring energy release in the Sun's atmosphere

该项目将探索太阳耀斑引起的太阳大气层中的快速能量释放。该项目将利用对太阳的最新X射线和其他多波长观测，探测太阳耀斑，特别是较小但频率很高的微耀斑的加热和粒子加速性质。将使用最新的分析技术，并将使用能量释放的衍生物理特性来驱动模型和模拟。这项工作将有助于我们进一步了解太阳大气是如何被加热的，以及这种脉冲能量释放背后的物理过程。

This project will explore the rapid energy release in the Sun's atmosphere due to solar flares. Using the latest X-ray and other multi-wavelength observations of the Sun, this project will probe the nature of heating and particle acceleration in solar flares, particularly the smaller but highly frequent microflares. The latest analysis techniques will be used, and the derived physical properties of the energy release will be used to drive models and simulations. This work will help further our understanding of how the solar atmosphere is heated, and the physical processes behind this impulsive energy release.