Source functions in the cores of infrared Fraunhofer lines
β Scribed by C. Jager; L. Neven
- Publisher
- Springer
- Year
- 1968
- Tongue
- English
- Weight
- 152 KB
- Volume
- 3
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
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
Absolute wavelengths for Fraunhofer lines are compared with laboratory measurements for several atomic and molecular spectra. The wavelength differences are shown to be consistent with the proposal that the deeper layers of the photosphere are in convective motion: ve -~ 3 km/sec for log To> --1.0.