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Solar brightness distribution at 8.6 mm from interferometer observations
Authors:K. Kawabata  M. Fujishita  T. Kato  H. Ogawa  T. Omodaka
Affiliation:(1) Department of Physics and Astrophysics, Nagoya University, Chikusa-ku Nagoya, Japan
Abstract:The radial brightness distribution of the quiet Sun at 8.6 mm is synthesized from observations using a sixteen element east-west interferometer in Nagoya. The observed brightness is flat from the disk center to 0.8Rodot. A slight darkening appeared between 0.8Rodot and the limb. No evidence of the bright ring near the limb is found. The radio radius at 8.6 mm is 1.015±0.005Rodot. In addition there exists a coronal component just outside the radio limb.
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