Data files used in real-time Solar Orbiter predictions

Processed data files used for real-time CME prediction codes. Solar Orbiter files are in RTN coordinates, and have been made into pickle files using datafiles provided directly by the Imperial College London Solar Orbiter MAG team. NOAA real-time magnetic field data is in GSM coordinates. Taken directly from https://services.swpc.noaa.gov/products/solar-wind/ at the time and saved as pickle files. NOAA real-time Dst index files are taken from https://services.swpc.noaa.gov/products/kyoto-dst.json and also saved as pickle files. Predicted SYM-H files are the output from the Temerin &amp; Li model. <br>

本数据集为用于实时日冕物质抛射（Coronal Mass Ejection, CME）预测代码的预处理数据文件。太阳轨道飞行器（Solar Orbiter）相关数据采用径向-切向-法向（Radial-Tangential-Normal, RTN）坐标系，其数据源自伦敦帝国理工学院太阳轨道飞行器磁强计（Magnetometer, MAG）团队直接提供的原始文件，并已封装为pickle格式文件（pickle）。美国国家海洋和大气管理局（National Oceanic and Atmospheric Administration, NOAA）实时磁场数据采用地心太阳磁层（Geocentric Solar Magnetospheric, GSM）坐标系，该数据于对应采集时段直接从https://services.swpc.noaa.gov/products/solar-wind/ 获取，并保存为pickle格式文件（pickle）。NOAA实时Dst指数文件源自https://services.swpc.noaa.gov/products/kyoto-dst.json，同样保存为pickle格式文件（pickle）。SYM-H指数预测文件为特梅林与李（Temerin & Li）模型的输出结果。