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Complete Alpha-Tensor for Solar Dynamo

Published online by Cambridge University Press:  19 July 2016

V.N. Krivodubskij and
M. Schultz
V.N. Krivodubskij
Affiliation:
Astronomical Observatory of Kiev University, Kiev 254053, Ukraine
M. Schultz
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, Potsdam D-O-1591, Germany

Abstract

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We applied the results of recent derivations of the α-effect to the solar convection zone model by Stix (1989) to find the depth and latitude dependences of the α-tensor. Pronounced inhomogeneity and anisotropy are revealed: the α-coefficients for different directions are quite different and strongly latitude-dependent.

Information

Type
1. The Solar Dynamo
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993, pp. 25 - 26
Copyright
Copyright © Kluwer 1993 

References

Elstner, D. and Rüdiger, G.: 1993, This volume Google Scholar
Rüdiger, G. and Kichatinov, L.L.: 1993 Astron. Astrophys. (in press) Google Scholar
Stix, M.: 1989, The Sun: An Introduction , Springer, Berlin Heidelberg Google Scholar