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Observations of prominences at 3.5 millimeter wavelength
Authors:M R Kundu
Institution:(1) Astronomy Program, University of Maryland, College Park, Md., U.S.A.
Abstract:At 3.5 mm wavelength absorption features are observed in correspondence with Hagr dark filaments on the disk; beyond the limb the prominences correspond to emissive regions. The absorption features are larger (2prime–3prime arc) than the corresponding Hagr dark filaments; the emissive regions at the limb have similar angular sizes. The emissive regions at the limb have electron temperatures of 5500±500 K; the amount of absorption observed on the disk leads to mean electron densities of about 5 × 1010 per cm3.
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