Kinematic dynamo wave in the vicinity of the solar poles

Details Kinematic dynamo wave in the vicinity of the solar poles Kinematic dynamo wave in the vicinity of the solar poles

2001-04-27

arxiv.org/abs/astro-ph/0104444v1

Geophys. Astrophys. Fluid Dynamics, Vol. 91, pp. 147-167 (1999)

Astronomy and Astrophysics

Astrophysics

20 pages, 2 EPS figures

Scientific paper

10.1080/03091929908203702

We consider a dynamo wave in the solar convective shell for the kinematic $\alpha\omega$-dynamo model. The spectrum and eigenfunctions of the corresponding equations are derived analytically with the aid of the WKB method. Our main aim here is to investigate the dynamo wave behavior in the vicinity of the solar poles. Explicit expressions for the incident and reflected waves are obtained. The reflected wave is shown to be relatively weak in comparison to the incident wave. The phase shifts and the ratio of amplitudes of the two waves are found.

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