Ya-Hui Yang

(National Central University)

Solar flare is one of the most explosive phenomena in solar system that huge energy is released in a short time and radiation is emitted almost across the entire electromagnetic spectrum. In particular, the radio emission is associated with the particle acceleration process in the corona, as well as the transportation process in the lower solar atmosphere or interplanetary space, and thus can provide important information on the acceleration and transport processes of non-thermal electrons in solar flares and coronal mass ejections (CMEs). Students in the summer program will analyze the properties of solar type II and type III radio bursts, which are produced by the CME-driven shock and magnetic reconnection, based on the ground-basedradio measurements.In addition to the data analysis, students can learn the magnetic reconnection and particle acceleration theories related to the solar eruptive events.