The brightness distribution near the solar limb has been investigated by means of a technique in which derivatives of drift scans of the Sun were compared with derivatives of drift scans of the Moon. The results obtained at 88.3 GHz (3.4 ram) indicate that the Sun is limb neutral within the uncertai
โฆ LIBER โฆ
Solar brightness distribution and its variability at 3 millimeter wavelength
โ Scribed by V. G. Nagnibeda; V. V. Piotrovitch
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 345 KB
- Volume
- 152
- Category
- Article
- ISSN
- 0038-0938
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