NAU Harvester System
Double maxima of 11-year solar cycles
Вісник астрономічної школи
View Archive Info| Field | Value | |
| Title |
Double maxima of 11-year solar cycles
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| Creator |
Krivodubskij V.N.
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| Date |
2015
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| Source |
Astronomical School’s Report, 2015, Volume 11, Issue 1, P. 34-47
2411-6602 |
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| Identifier |
http://astro.nau.edu.ua/papers/AstSR_2015_Vol_11_Iss_1_P_34.pdf
10.18372/2411-6602.11.1034 |
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| Language |
uk
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| Description |
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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| Publisher |
National Aviation University
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| Format |
application/pdf
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