演講資訊

摘要：

Solar flares and coronal mass ejections are two major eruptive phenomena of solar storms. The accompanied radiations and energetic particles can cause space weather events in the solar-terrestrial environment. Since radio emissions, particularly the solar radio bursts, are produced by the accelerated electrons from solar explosions when the electrons transport outward along open magnetic fields through the corona and interplanetary space, radio wave is regarded as a good diagnostic tool to investigate the dynamic properties of electron beams and ambient medium. In this talk, I will briefly introduce the solar radio observations and the related space weather effects. Then I will focus on the study of type III solar radio burst detected by Parker Solar Probe spacecraft and show you the monitor of solar radio bursts at Taiwan-NCU station in the end.