2021
DOI: 10.1007/s11207-020-01745-6
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The Fine Structure of the Quasi-Biennial Oscillations of Sunspot Areas and the Double Magnetic Cycle of the Sun

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Cited by 3 publications
(3 citation statements)
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“…Around the maxima of the two cycles, modulations at lower frequencies are visible between 500 and 1500 days and can be interpreted as the manifestation of the quasi-biennal oscillation in sunspot coverage (e.g. Kostyuchenko & Bruevich 2021). The reconstructed spot coverage exhibits similar features, although some discrepancies are also visible.…”
Section: A Difficult Case With Ground Truth: the Sunmentioning
confidence: 92%
“…Around the maxima of the two cycles, modulations at lower frequencies are visible between 500 and 1500 days and can be interpreted as the manifestation of the quasi-biennal oscillation in sunspot coverage (e.g. Kostyuchenko & Bruevich 2021). The reconstructed spot coverage exhibits similar features, although some discrepancies are also visible.…”
Section: A Difficult Case With Ground Truth: the Sunmentioning
confidence: 92%
“…In addition, the featured coronal holes and sunspots determine the solar cycle and the three-dimensional (3D) heliospheric magnetic configuration that establishes the Sun-heliosphere connection. In this respect, within this collection, fundamental investigations have been performed to understand the solar atmosphere plasma thermodynamics, magnetic field configuration, and long-term variations (Lloveras et al, 2020;Ryabov and Vrublevskis, 2020;Kostyuchenko and Bruevich, 2021;Nandy, 2021). Lloveras et al (2020) carried out, compared, and reported a detailed study of the global 3D structure of the electron density and temperature of the quiescent inner solar corona based on the differential emission measure tomography (DEMT) and the Alfvén Wave Solar Model (AWSoM) in their latest versions.…”
mentioning
confidence: 99%
“…This is another noteworthy contribution to this TC. In the study carried out by Kostyuchenko and Bruevich (2021), the authors focused on the fine structure of quasi-biennal oscillations (QBOs) of the sunspot areas during Solar Cycles 19 -23. The QBO period gradually decreases from the beginning of the solar cycle till the end in phase with the shift of the average latitudes of sunspots to the equator: a scenario of this behavior within the convection zone is proposed.…”
mentioning
confidence: 99%