The OSO-8 satellite enabled us to study various characteristics of the profiles of Si 1I, Si Iv, C IV, and O Vl lines above active areas of the Sun, as well as above quiet areas, and to derive some physical properties of the transition region between chromosphere and corona (CCT): (i) The study of t
โฆ LIBER โฆ
Structure and physics of solar faculae
โ Scribed by J. -C. Pecker; S. Dumont; Z. Mouradian
- Publisher
- Springer
- Year
- 1992
- Tongue
- English
- Weight
- 974 KB
- Volume
- 138
- Category
- Article
- ISSN
- 0038-0938
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