arXiv · 1904.05826
Radio, Millimeter, and Sub-millimeter Observations of the Quiet Sun
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.
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Tim Bastian, Bin Chen, Dale Gary, Gregory Fleishman, Lindsay Glesener, Colin Lonsdale, Pascal Saint-Hilaire, Stephen White. 2019-04-11. Radio, Millimeter, and Sub-millimeter Observations of the Quiet Sun. https://arxiv.org/abs/1904.05826
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