Studies on the Temperature Structure and Heating of the Solar Corona by Solar-B and Solar Magnetic Activity Research Telescope (SMART)

摘要

In this paper, we discuss the coordinated observation by Solar-B and Solar Magnetic Activity Research Telescope (SMART) for the coronal heating study. The high time cadence wide field of view vector magnetic field maps obtained by SMART will be essential for the large scale magnetic field evolution and its relationship to the coronal heating.