The oscillatory behaviour of solar faculae
โ Scribed by H. Balthasar
- Publisher
- Springer
- Year
- 1990
- Tongue
- English
- Weight
- 156 KB
- Volume
- 127
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
Tile oscillatory behaviour of some faculae has been observed. In some cases power values in the faculae are larger than in the photosphere, but in other faculae power minima are found.
๐ SIMILAR VOLUMES
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
Theories of solar flares based on the storage of energy (usually as magnetic energy) in the solar atmosphere are shown to be incompatible with observational data. The sunspot energy deficit and the photospheric faculae both involve energy fluxes comparable with the flare requirement ( ~ 3 โข 1029 er
Comparison of the long-term variation of photospheric faculae areas with that of sunspots shows that studies of faculae provide both complementary and supplementary information on the behaviour of the solar cycle. Detailed studies of the development of sunspots with respect to faculae show that ther