Consolidated Solar and Heliospheric Physics Research at UCLan

这项综合赠款提案将在中央兰开夏大学耶利米·霍罗克斯研究所的太阳物理组内开展的研究项目集中在一起。这些项目旨在研究太阳的外层大气、日冕及其相关结构，如活动区和日冕环。太阳活动，包括太阳耀斑和日冕物质抛射(日冕物质抛射)以及相关的高能粒子也是研究的重点。调查将包括：-分析太阳黑子的自转是否能够提供足够的能量来驱动太阳活动区及其相关活动，如太阳耀斑和日冕物质抛射。-利用美国宇航局高分辨率日冕成像仪(Hi-C)和欧空局的太阳轨道飞行器任务的高分辨率数据，结合理论模型，研究太阳活动区的日冕环特征。-通过将模拟结果与帕克太阳探测器和太阳轨道飞行器在靠近太阳的空间位置进行的数据进行比较，分析太阳高能粒子在耀斑和日冕物质抛射期间如何加速以及它们如何在太空中传播。

This consolidated grant proposal groups together research projects to be carried out within the Solar Physics group of the Jeremiah Horrocks Institute at the University of Central Lancashire. The projects aim to study the outer atmosphere of the Sun, the solar corona, and its associated structures, such as active regions and coronal loops. Solar activity, including solar flares and Coronal Mass Ejections (CMEs) and the associated energetic particles are also a focus of the research. The investigations will include:- analysing whether the rotation of sunspots can provide sufficient energy to power solar active regions and their associated activity, such as solar flares and CMEs.- studing coronal loops, characteristic of solar active regions, by using high-resolution data from NASA's High resolution Coronal Imager (Hi-C) and ESA's Solar Orbiter mission combined with theoretical models.- analysing how Solar Energetic Particles are accelerated during flares and CMEs and how they propagate through space, by comparing simulation results with data from the Parker Solar Probe and Solar Orbiter missions taken at locations in space near the Sun.