In a spectrogram of exceptionally high spatial resolution, brightness and velocity fluctuations in seven weak to medium-strong Fe I lines have been measured and analyzed. Heights of formation of these lines have been computed using the Harvard-Smithsonian Reference Atmosphere (Gingerich et al., 1972
The characteristic size and brightness of facular points in the quiet photosphere
β Scribed by Richard Muller; Stephen L. Keil
- Publisher
- Springer
- Year
- 1983
- Tongue
- English
- Weight
- 536 KB
- Volume
- 87
- Category
- Article
- ISSN
- 0038-0938
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