Radio, Millimeter, and Sub-millimeter Observations of the Quiet Sun
Solar and Stellar Astrophysics
2019-04-12 v1
Abstract
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.
Keywords
Cite
@article{arxiv.1904.05826,
title = {Radio, Millimeter, and Sub-millimeter Observations of the Quiet Sun},
author = {Tim Bastian and Bin Chen and Dale Gary and Gregory Fleishman and Lindsay Glesener and Colin Lonsdale and Pascal Saint-Hilaire and Stephen White},
journal= {arXiv preprint arXiv:1904.05826},
year = {2019}
}
Comments
White paper submitted to the Astronomy and Astrophysics decadal survey