A method for the evaluation of the brightness distribution in the solar corona
โ Scribed by W. Stanek
- Publisher
- Springer
- Year
- 1971
- Tongue
- English
- Weight
- 329 KB
- Volume
- 21
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
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
An improved value of coronal temperature is obtained by the degree of ionization method taking various processes into consideration. Comparison with some of the existing results has also been made. The problem of establishing the temperature distribution in solar corona has been of interest to many