Global modes constituting the solar magnetic cycle. II - Phases, 'geometrical eigenmodes', and coupling of field behaviour in different latitudes

Physics

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Magnetohydrodynamics, Solar Cycles, Solar Magnetic Field, Solar Oscillations, Solar Spectra, Statistical Distributions, Sunspots, Superhigh Frequencies

Scientific paper

The information present in the computed phases of the SHF modes of the sun spectrum is used to identify four independent geometrical modes of coherent global oscillations ('geometrical eigenmodes') in the field. It is shown that these geometrical eigenmodes represent physically global oscillations actually existing in the sun's magnetic field. The combination of the four coherent oscillations is sufficient to reproduce not only the observed behavior of the real field in the low latitudes, but also its couplings to the behavior in the middle and the high latitudes.

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