Excitation of non-axially symmetric modes of the Sun's mean magnetic field |
| |
| Authors: | A. A. Ruzmaikin D. D. Sokoloff S. V. Starchenko |
| |
| Affiliation: | (1) Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, SU-142092 Troitsk, Moscow Region, U.S.S.R.;(2) Moscow State University, 119899 Moscow, LenGory, U.S.S.R.;(3) Lenin State Pedagogical Institute, Moscow, U.S.S.R. |
| |
| Abstract: | The kinematic dynamo equations for the mean magnetic field are solved with an asymptotic method of the WKB type. The excitation conditions and main characteristics of the non-axially symmetric modes for a given distribution of the sources are obtained. Utilization of the helioseismologic data on the Sun's internal rotation permits an explanation, within the framework of dynamo theory, of the excitation of the main non-axially symmetric modes revealed in the Sun's magnetic field sector structure. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
