Development of a Polarimeter System for Solar Synoptic High-Sensitivity Observations
Solar activities are dominated by magnetic fields. Solar Coronal Mass Ejections (CMEs) are often associated with pre-existing filaments or prominences. The determination of the magnetic field in the solar chromosphere before, during, and after a CME event will allow us to derive the conditions that trigger CMEs and the magnetic field properties of the ejected material. Both ingredients are crucial to improve the...