Abstract
A synthesis of the centimetric and millimetric observations of the prominences on the disk is performed using the published radio maps as well as original observations. It is shown that the size of the radio depressions associated with large quiescent Hα filaments is similar to the Hα size. A spectrum of the brightness temperature of the radio filaments between 3.5 mm and 6 cm-λ is derived.
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Raoult, A., Lantos, P. & Fürst, E. Prominences at centimetric and millimetric wavelengths. Sol Phys 61, 335–343 (1979). https://doi.org/10.1007/BF00150418
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DOI: https://doi.org/10.1007/BF00150418