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 3mm wavelength from observations of the eclipse of 1976 October 23
โ Scribed by N. R. Labrum; J. W. Archer; C. J. Smith
- Publisher
- Springer
- Year
- 1978
- Tongue
- English
- Weight
- 642 KB
- Volume
- 59
- Category
- Article
- ISSN
- 0038-0938
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