This contribution is a purely exploratory search to investigate the way the distribution of angular velocity inside the Sun's convection zone affects the energy transport. This is related with problems concerning the magnetic activity, whose appearance at the Sun's surface depends on the shape of th
β¦ LIBER β¦
Observations of longperiod mass velocity oscillations in the Sun's chromosphere
β Scribed by V. S. Bashkirtsev; N. I. Kobanov; G. P. Mashnich
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 418 KB
- Volume
- 109
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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