Eigenvectors of solar magnetic field in cycles 21-24 and their links to solar activity indices

Using full disc synoptic maps of solar background magnetic field captured from the Wilcox Solar Observatory for 30 latitudinal bands for cycles 21-24, principal components (PCs) or eigenvectors of magnetic oscillations are obtained. The PCs are shown to come in pairs assigned to magnetic waves produ...

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Bibliographic Details
Main Authors: Shepherd, S.J (Author), Zharkova, V.V (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
Subjects:
Online Access:View Fulltext in Publisher
LEADER 03004nam a2200385Ia 4500
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020 |a 00358711 (ISSN) 
245 1 0 |a Eigenvectors of solar magnetic field in cycles 21-24 and their links to solar activity indices 
260 0 |b Oxford University Press  |c 2022 
856 |z View Fulltext in Publisher  |u https://doi.org/10.1093/mnras/stac781 
520 3 |a Using full disc synoptic maps of solar background magnetic field captured from the Wilcox Solar Observatory for 30 latitudinal bands for cycles 21-24, principal components (PCs) or eigenvectors of magnetic oscillations are obtained. The PCs are shown to come in pairs assigned to magnetic waves produced by dipole, quadruple, sextuple, and octuple magnetic sources. The first pair is linked to dipole magnetic waves with their summary curve revealing a reasonable fit to the averaged sunspot numbers in cycles 21-24. This verifies the previous results and confirms the summary curve as additional proxy of solar activity decreasing towards grand solar minimum in cycles 25-27. There is also a noticeable asymmetry in latitudinal distributions of these PCs showing an increased activity in Northern hemisphere in odd cycles and in Southern hemisphere in even ones similar to the N-S asymmetries observed in sunspots. The second pair of PCs linked to quadruple magnetic sources has 50 per cent smaller amplitudes than the first, while their summary curve correlates closely with soft X-ray fluxes in solar flares. Flare occurrences are also linked to variations of the next two pairs of eigenvectors, quadruple and sextuple components, revealing additional periodicity of about 2.75-3.1 yr similar to observed oscillations in flares. Strong latitudinal asymmetries in quadruple and sextuple components are correlating with the N-S asymmetries of flare occurrences skewed to Southern hemisphere in even cycles and to Northern hemisphere in odd ones. Principal component analysis of solar magnetic field raises perspectives for simultaneous prediction of general and flaring solar activity. © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. 
650 0 4 |a Eigenvalues and eigenfunctions 
650 0 4 |a Flare 
650 0 4 |a flares 
650 0 4 |a Magnetic fields 
650 0 4 |a Magnetic waves 
650 0 4 |a Methods. Data analysis 
650 0 4 |a methods: data analysis 
650 0 4 |a methods: miscellaneous 
650 0 4 |a Methods: miscellaneous 
650 0 4 |a Principal component analysis 
650 0 4 |a Principal Components 
650 0 4 |a Solar energy 
650 0 4 |a Solar magnetic fields 
650 0 4 |a Solar radiation 
650 0 4 |a Summary curve 
650 0 4 |a Sun: activity 
650 0 4 |a Sun: magnetic field 
650 0 4 |a Sun:magnetic fields 
650 0 4 |a Sunspot 
650 0 4 |a sunspots 
700 1 |a Shepherd, S.J.  |e author 
700 1 |a Zharkova, V.V.  |e author 
773 |t Monthly Notices of the Royal Astronomical Society