We discuss a recent model for the solar chromosphere proposed by Suemoto (Solar Phys. 54, 3). We conclude that the model is incompatible with the basic constraints imposed by high resolution observations and by line formation theory, and that consequently the model does not adequately describe the s
An empirical, statistical model for the formation of the cores of chromospheric Fraunhofer lines
β Scribed by Z. Suemoto
- Publisher
- Springer
- Year
- 1977
- Tongue
- English
- Weight
- 1002 KB
- Volume
- 54
- Category
- Article
- ISSN
- 0038-0938
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