DynaSun - Dynamics Of The Solar Corona In The Era Of Data Intensive Observations

DynaSun - 数据密集观测时代的日冕动力学

• 批准号: EP/Y037464/1
• 负责人: James McLaughlin
• 金额: $ 21.84万
• 依托单位: Northumbria University
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2024
• 资助国家: 英国
• 起止时间: 2024 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=EP%2FY037464%2F1
• 关键词: DynaSun; Dynamics; Solar; Corona; Era

The aim of this proposal is to establish close research collaboration between several leading European and South American research teams specialising in solar physics; and gain new, paradigm-changing knowledge about dynamic processes in the solar atmosphere, through the systematic research staff and knowledge exchange and joint research efforts exploiting existing data and facilities, including innovative data analysis techniques based on the machine-learning approach.The expected scientific impact is a major development of our knowledge of the key physical processes operating in the solar atmosphere, including breakthroughs in revealing the coronal heating mechanism, transformative progress in our understandingimpulsive energy realises such as solar flares and CMEs, major development of MHD wave theory, and first application of machinelearning techniques in the study of solar atmospheric wave processes. The project includes four scientific work packages whichaddress specific key challenges of modern solar physics and heliophysics: quasi-periodic pulsations in solar flares, heating of the solar atmosphere, and large and fine scale evolution of CMEs, and a communication and dissemination work package. The expectedeconomic and technological impacts include gaining first-hand experience in the analysis of complex oscillatory processes, experience in designing and applying machine-learning techniques for pattern recognition, novel diagnostic techniques of inputparameters for space weather forecasting models, creating a ground for knowledge exchange with local industries, and production of highly-skilful specialists in numerical modelling and data analysis. The expected societal impact is strengthening the research links between the European and S. American research communities;

该提案的目的是建立几个专门从事太阳能物理学的欧洲和南美领先的研究团队之间的密切研究合作。并通过系统的研究人员和知识交流和共同的研究工作来获得有关太阳大气中动态过程的新的，改变范式的知识意识到诸如太阳耀斑和CME，MHD波理论的主要发展以及在太阳大气波过程研究中的首次应用机械学习技术。该项目包括四个科学工作包，这些工作包使现代太阳能物理和热物理学的特定主要关键挑战：太阳耀斑中的准周期性脉动，太阳能大气的加热以及CMES的大型演变，以及通信和传播工作包。预期的经济和技术影响包括在分析复杂振荡过程中获得第一手经验，在设计和应用机器学习技术方面的经验，用于模式识别的新型诊断技术的新型诊断技术，用于太空天气预测模型，为当地行业提供知识交换的基础，并在数字模型和数据分析中创造了知识交换的基础。预期的社会影响正在加强欧洲和美国研究社区之间的研究联系；