http://arxiv.org/abs/1904.05826
Identification of the mechanisms responsible for heating the solar chromosphere and corona remains an outstanding problem, one of great relevance to late-type stars as well. There has been tremendous progress in the past decade, largely driven by new instruments, new observations, and sophisticated modeling efforts. Despite this progress, gaps remain. We briefly discuss the need for radio coverage of the 3D solar atmosphere and discuss the requirements.
T. Bastian, B. Chen, D. Gary, et. al.
Fri, 12 Apr 19
2/62
Comments: White paper submitted to the Astronomy and Astrophysics decadal survey