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Queen's University Belfast Consolidated Grant in Solar Physics and Solar System Studies 2017 - 2020

贝尔法斯特女王大学太阳物理和太阳系研究综合补助金 2017 - 2020

基本信息

批准号：
ST/P000304/1
负责人：
Francis Keenan
金额：
$ 166.6万
依托单位：
Queen's University Belfast
依托单位国家：
英国
项目类别：
Research Grant
财政年份：
2017
资助国家：
英国
起止时间：
2017 至无数据
项目状态：
已结题

来源：
https://gtr.ukri.org/projects?ref=ST%2FP000304%2F1
关键词：
Queen University Belfast Consolidated Grant

项目摘要

Our Consolidated Grant brings together research projects in solar physics, and the study of solar system bodies, undertaken by staff within the School of Mathematics and Physics at Queen's University Belfast. All of these projects fall within the remit of the Solar Studies (SS) and Planetary Studies (PL) sub-panels of the STFC Astronomy Grants Panel. The programme is diverse, with the solar physics projects involving observational and computational studies of the solar atmosphere from the chromosphere to the corona, with a particular emphasis on high-frequency imaging and spectroscopy of dynamic events, including wave generation, propagation and dissipation, the cancellation of magnetic elements and total solar eclipses. Projects on solar system bodies include observational studies of asteroids and the most primitive populations such as comets/trans-Neptunian objects - populations that retain key information on the origin and evolution of our planetary system. Our observational research employs an extensive set of both ground- and satellite-based solar and astronomical facilities, including the ROSA/HARDcam high-cadence solar imager, the Pan-STARRS Survey, ESO, ING and Gemini telescopes, and the SDO and Hinode satellites. In addition, we use the DiRAC supercomputing facility to support the computational aspects of our research programmes.

我们的综合赠款将由贝尔法斯特女王大学数学和物理学院的工作人员负责的太阳物理研究项目和太阳系天体研究结合在一起。所有这些项目都属于STFC天文学补助金小组的太阳研究(SS)和行星研究(PL)小组的职权范围。方案是多样的，太阳物理项目涉及对从色球到日冕的太阳大气层的观测和计算研究，重点是动态事件的高频成像和光谱，包括波的产生、传播和消散、磁元素的抵消和日全食。关于太阳系天体的项目包括对小行星和最原始种群的观测研究，如彗星/跨海王星天体--这些种群保留了关于我们行星系统起源和演化的关键信息。我们的观测研究使用了一套广泛的地面和卫星太阳和天文设施，包括ROSA/HARDcam高频率太阳成像仪、泛星观测、欧洲南方天文台、ING和双子座望远镜，以及SDO和Hinode卫星。此外，我们使用DIRAC超级计算设施来支持我们研究计划的计算方面。