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Identification of the mechanisms responsible for heating the solarchromosphere and corona remains an outstanding problem, one of great relevanceto late-type stars as well. There has been tremendous progress in the pastdecade, largely driven by new instruments, new observations, and sophisticatedmodeling efforts. Despite this progress, gaps remain. We briefly discuss theneed for radio coverage of the 3D solar atmosphere and discuss therequirements.

Radio, Millimeter, and Sub-millimeter Observations of the Quiet Sun