Consolidated Solar System Physics Research at UCLan

这项综合拨款提案汇集了中央兰开夏大学（UCLan）耶利米霍罗克斯研究所（JHI）的研究成果，以及与开放大学研究人员在太阳和日球层物理学研究领域的合作。在这些领域，我们将在太阳系研究的前沿解决关键科学问题，即太阳动力学及其对当地环境的影响。具体项目包括：-研究太阳黑子旋转对太阳活动（如太阳耀斑和日冕物质抛射）的影响，以确定太阳黑子旋转是否会导致太阳活动增加；-利用magexs探空火箭飞行数据和Hinode卫星上的EIS仪器探索日冕环加热的本质，以约束理论和数值加热模型；-确定太阳大气层不同层的情况如何影响日冕物质抛射的发生，以及大气变暗是否可以用作预测日冕物质抛射的诊断指标；-用数值代码模拟太阳高能粒子（sep）在内日球层的传播，并与观测结果进行比较，以确定整个太阳系的潜在物理特性；-绘制水星附近的黄道云，以更好地了解尘埃对该行星的影响，并将黄道云作为一个整体进行测量，以调查行星对云和行星际尘埃来源的影响。

This consolidated grant proposal brings together research within the Jeremiah Horrocks Institute (JHI) of the University of Central Lancashire (UCLan), along with consortium collaboration with researchers at the Open University, in the research areas of solar and heliospheric physics. In these areas we will be addressing key science questions at the cutting edge of solar system research about the dynamics of the Sun and how it effects it local environment. Specific projects include:- investigating the effect of the rotation of sunspots on solar activity such as solar flares and coronal mass ejections to determine whether sunspot rotation leads to increased solar activity; - exploring the nature of coronal loop heating using data from the MaGIXS sounding rocket flight and the EIS instrument on the Hinode satellite to constrain theoretical and numerical heating models; - determining how conditions in the different layers of the Sun's atmosphere influence the onset of coronal mass ejections (CMEs), and whether atmospheric dimmings can be used as a diagnostic to predict CMEs; - modelling the propagation of Solar Energetic Particles (SEPs) in the inner heliosphere with numerical codes and comparing with observations to determine the underlying physics throughout the solar system; - mapping the zodiacal cloud near Mercury to better understand dust impacts on that planet, and, surveying the zodiacal cloud as a whole to investigate the effects of planets on the cloud and the sources of interplanetary dust.