Double maxima of 11-year solar cycles
The explanation of the observed phenomenon of double peaks of the 11 year sunspot cycles is proposed. The scenario involves five processes of reconstruction of magnetism in the solar convective zone (SCZ): ω effect, magnetic buoyancy, macroscopic turbulent diamagnetism, rotary ∇ρ effect and meridion...
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| Format: | Article |
| Language: | English |
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National Aviation University
2015-10-01
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| Series: | Вісник Астрономічної школи |
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| Online Access: | http://astro.nau.edu.ua/issues/2015_V.11_Iss.1/Krivodubskij.html |
| Summary: | The explanation of the observed phenomenon of double peaks of the 11 year sunspot cycles is proposed. The scenario involves five processes of reconstruction of magnetism in the solar convective zone (SCZ): ω effect, magnetic buoyancy, macroscopic turbulent diamagnetism, rotary ∇ρ effect and meridional circulation. It was established that the reconstruction of magnetism in high-latitude and equatorial domains of the SCZ occurs in different modes. Two time-shifted waves of the toroidal field to the solar surface play a key role in the proposed mechanism in the equatorial domain. |
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| ISSN: | 1607-2855 2411-6602 |