Collaborative Research: SHINE--Automated System for Observation-Based Real-Time Simulation of the Solar Corona and Inner Heliosphere at the Community Coordinated Modeling Center

研究人员将开发一个自动化系统，用于在社区协调建模中心（CCMC）持续运行基于研究的，观测驱动的，实时模拟日冕和内日光层。每天或更频繁地，系统将使用最新的太阳磁象作为输入，并将上次模拟的结果作为新模拟的初始条件，自动重新启动新的日冕状态模拟。预测整个日冕和日光层内的行星际磁场和太阳风参数的三维和随时间变化的分布是空间物理学中最具挑战性的科学问题之一。如果每天例行实时进行模拟，并将最新的磁测图数据作为模型的输入，同时有能力利用连续不断的观测数据来验证模型，则这项任务就变得更加困难。空间气象建模框架（SWMF）的太阳日冕模型，已经在CCMC提供，将用于这项工作。为了验证该模型，将制作合成的极紫外线图像，与美国航天局卫星仪器观测到的图像进行比较。耦合模型预测将不断与ACE卫星测量的太阳风参数进行验证。该研究的智力价值是开发了一个基于研究的模型，该模型可用于更好地了解日冕物质抛射（CME）的传播，无论是在日冕图像中观察到CME签名时的实时，还是对有趣事件的历史分析和研究。该项目更广泛的影响是，将向CCMC提供新一代太阳-日光层系统全球模型，使太阳-太阳物理学界能够广泛使用。该项目将培训一名初级女博士后研究员，并将加强研究和教育基础设施。

The investigators will develop an automated system for continuously running a research-based, observation-driven, real-time simulation of the solar corona and inner heliosphere at the Community Coordinated Modeling Center (CCMC). Every day, or more frequently, the system will automatically restart a new simulation of the state of the solar corona using the latest solar magnetogram as the input and the result of the previous simulation as the initial condition for the new one. A prediction of the realistic three-dimensional (3D) and time-dependent distributions of the interplanetary magnetic field and solar wind parameters throughout the solar corona and inner heliosphere is one of the most challenging scientific problems in space physics. The task becomes even more difficult if the simulation is routinely performed in real-time, on a daily basis, with the latest magnetogram data incorporated as an input for the model together with the capability to validate the model using a continuous flow of observational data. The Space Weather Modeling Framework (SWMF) model of the solar corona, already available in the CCMC, will be used for the effort. To validate the model, synthetic extreme ultraviolet images will be produced to compare with the images as observed with NASA satellite instruments. The coupled model prediction will be continuously validated with the solar wind parameters measured by the ACE satellite. The intellectual merit of the research is the development of a research-based model that can be used to better understand the propagation of Coronal Mass Ejections (CMEs), both in real-time when CME signatures are observed in coronograph images, and for historical analysis and research of interesting events. The broader impact of the project is that a new generation of global models of the Sun-heliosphere system will be delivered to the CCMC to enable broad use by the solar-heliophysics community. The project will involve the training of a junior female postdoctoral researcher and will enhance infrastructure for research and education.