Fitting a modified ATLCW quiet-Sun model to ALMA, Metsähovi, and Nobeyama observations yields prominence densities 60-163 times higher and temperatures 155-163 times lower than the quiet Sun, with non-hydrostatic (magnetostatic) support favored.
(2019), Metsähovi Radio Observatory pub- lic solar database, Aalto University, Metsähovi Radio Obser- vatory.,http://urn.fi/urn:nbn:fi:att:f371cb6d-f84c -4d76-99e4-c39c639fd0de
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Modeling brightness temperature of prominences on the solar disk using ALMA single-dish observations
Fitting a modified ATLCW quiet-Sun model to ALMA, Metsähovi, and Nobeyama observations yields prominence densities 60-163 times higher and temperatures 155-163 times lower than the quiet Sun, with non-hydrostatic (magnetostatic) support favored.