✦ LIBER ✦

Global model of differential rotation in the Sun

✍ Scribed by Steven A. Balbus; Henrik Latter; Nigel Weiss

Book ID: 110093971
Publisher: John Wiley and Sons
Year: 2012
Tongue: English
Weight: 554 KB
Volume: 420
Category: Article
ISSN: 0035-8711
DOI: 10.1111/j.1365-2966.2011.20217.x

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📜 SIMILAR VOLUMES

On the sun's differential rotation

✍ B. R. Durney 📂 Article 📅 1974 🏛 Springer 🌐 English ⚖ 427 KB

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

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Differential rotation and magnetic torques in the interior of the Sun

✍ Rosner, R.; Weiss, N. O. 📂 Article 📅 1985 🏛 Nature Publishing Group 🌐 English ⚖ 371 KB

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Differential rotation and meridional circulation in global models of solar convection

✍ M.S. Miesch 📂 Article 📅 2007 🏛 John Wiley and Sons 🌐 English ⚖ 579 KB

Revealing of periodicities in the variat

Revealing of periodicities in the variations of differential rotation of the Sun

✍ M. Sh. Gigolashvili; N. A. Gogoladze; E. V. Khutsishvili 📂 Article 📅 1995 🏛 John Wiley and Sons 🌐 English ⚖ 593 KB

It is presumed that a north-southern asymmetry of a solid-body rotation of large spots, depending on even and odd solar activity cycles (Gigolashvili and Khutsishvilil 1989, 1990) may possibly be explained by the asymmetry of the appearance of large structures with strong magnetic fields in the corr

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Magnetic field and differential rotation in the radiative zone of the Sun

✍ R. N. Ikshanov; V. G. Ivanov 📂 Article 📅 1992 🏛 Springer 🌐 English ⚖ 554 KB

The problem of the interaction between magnetic fields and differential rotation in the radiative zone of the Sun is investigated. It is demonstrated that effects of magnetic buoyancy can be neglected in the analysis of this interaction. It is shown that hydromagnetic torsional waves propagating fro

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✍ L. L. Kichatinov 📂 Article 📅 1991 🏛 Springer 🌐 English ⚖ 841 KB

An axisymmetric model for the Sun's differential rotation based upon a mechanism for angular momentum transport by compressible convection is developed. Convective heat transport is also considered. The model is simplified by the neglect of meridional circulation and radiative heat transport but is