The brightness distribution of the quiet Sun at 8.6 mm wavelength is synthesized from off-meridian observations using an eight element east-west interferometer with a maximum base line of 16.38 m (1913A). The observed brightness distribution is practically flat from the disk center to the optical li
Solar brightness distribution at 8.6 mm from interferometer observations
โ Scribed by K. Kawabata; M. Fujishita; T. Kato; H. Ogawa; T. Omodaka
- Publisher
- Springer
- Year
- 1980
- Tongue
- English
- Weight
- 904 KB
- Volume
- 65
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
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 fiat from the disk center to 0.SR| A slight darkening appeared between 0.8R| and the limb. No evidence of the bright ring near the limb is found. The radio radius at 8,6 mm is 1.015 โข 0.005R| In addition there exists a coronal component just outside the radio limb.
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