Consolidated Solar System Physics Research at UCLan

这一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）内的研究，沿着与开放大学研究人员的财团合作，在太阳和日光层物理学的研究领域。在这些领域，我们将解决太阳系研究前沿的关键科学问题，即太阳的动力学及其如何影响当地环境。具体项目包括：调查太阳黑子旋转对太阳活动的影响，如太阳耀斑和日冕物质抛射，以确定太阳黑子旋转是否导致太阳活动增加;利用MaGIXS探空火箭飞行和Hinode卫星上的EIS仪器提供的数据探索日冕环加热的性质，以限制理论和数值加热模型;确定太阳大气层不同层的条件如何影响日冕物质抛射（CME）的发生，以及大气昏暗是否可以用作预测CME的诊断方法;- 用数字代码模拟太阳高能粒子在内日光层中的传播，并与观测结果进行比较，以确定整个太阳系的基本物理现象;绘制水星附近的黄道带云，以更好地了解尘埃对该行星的影响，对黄道光云进行整体观测，以研究行星对黄道光云的影响以及行星际尘埃的来源。

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.