It is assumed that the meridional motions (U) and angular velocity (g2) in the surface layers of the convection zone are given by simple expressions of the form: Ur=2~t(r)P2(cosO)/Qr 2, Uo = --~u'(r) sin0 cosO/er, and ~ =-(20[(1 + coo(r) + c02 (r) P2(cos0)]. Here q/(r) is the stream function, P2 (co
✦ LIBER ✦
Rotational evolution of the Sun
✍ Scribed by Nilgün Kiziloĝlu
- Publisher
- Springer Netherlands
- Year
- 1992
- Tongue
- English
- Weight
- 386 KB
- Volume
- 192
- Category
- Article
- ISSN
- 0004-640X
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