【科技日报】“羲和”号揭示太阳“暴脾气”的时序光谱特征

Core Insights - A research team from the Chinese Academy of Sciences, Zijinshan Observatory, and Nanjing University successfully analyzed solar eruption processes using the "Xihe" satellite, providing key insights into the physical processes of solar activity and their spectral characteristics [1][2] Group 1: Research Findings - The study focused on five different types of solar eruption events observed by the "Xihe" satellite in 2024, revealing distinct temporal spectral features associated with various physical processes of solar eruptions [2] - The analysis showed that in the flare region, the spatially integrated Hα spectrum exhibited continuous line center radiation enhancement, spectral line broadening, and red wing asymmetry, corresponding to the chromosphere compression process [2] - The research documented the evolution of solar dark filaments, showing changes in the spatially integrated Hα spectrum from accelerated blue shift absorption to decelerated blue shift absorption, and finally to red shift absorption, capturing the dynamics of cold plasma in dark filaments [2] Group 2: Scientific Significance - The findings highlight the scientific value of the "Xihe" satellite in comparative studies of solar and stellar atmospheric eruption activities, providing a unique opportunity to understand the origins and developments of such phenomena in other star-planet systems [1][2]