Solar brightness distribution at 8.6 MM from interferometer observations

Details Solar brightness distribution at 8.6 MM from interferometer observations Solar brightness distribution at 8.6 MM from interferometer observations

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...65..221k&link_type=abstract

Solar Physics, vol. 65, Mar. 1980, p. 221-227. Ministry of Education

Physics

7

Brightness, Interferometry, Solar Radio Emission, Stellar Luminosity, Data Reduction, Limb Darkening, Millimeter Waves, Radial Distribution, Solar Instruments, Weighting Functions

Scientific paper

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 0.8 earth radii. A slight darkening appeared between 0.8 earth radii and the limb. No evidence of the bright ring near the limb is found. The radio radius at 8.6 mm is 1.015 plus or minus 0.0005 earth radii. In addition there exists a coronal component just outside the radio limb.

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