2017/07/26 by Eka Gurgenashvili, T. V. Zaqarashvili, Teimuraz V. Zaqarashvili +8 · 63 citations
Biochemistry, Genetics and Molecular Biology · Physics and Astronomy · #Astro and Planetary Science #Astronomy #Astrophysics #Asymmetry #Atmospheric sciences #Climatology #Dynamo #Dynamo theory #Geology #Geomagnetism and Paleomagnetism Studies #Magnetic field #Northern Hemisphere #Physics #Rossby wave #Solar and Space Plasma Dynamics #Solar cycle #Solar dynamo #Solar wind #Southern Hemisphere #Sunspot #astro-ph.SR
paper · pdf · doi:10.3847/1538-4357/aa830a
published in The Astrophysical Journal 845(2), 137 (IOP Publishing) · 22 pages, 7 figures
arxiv created 2017/07/26 · openalex created_date 2017/08/08 · openalex publication_date 2017/08/18 · arxiv updated 2017/08/30 · openalex updated_date 2026/08/06
Abstract Rieger-type periodicity has been detected in different activity indices over many solar cycles. It was recently shown that the periodicity correlates with solar activity having a shorter period during stronger cycles. Solar activity level is generally asymmetric between northern and southern hemispheres, which could suggest the presence of a similar behavior in the Rieger-type periodicity. We analyze the sunspot area/number and the total magnetic flux data for northern and southern hemispheres during solar cycles 19–23, which had remarkable north–south asymmetry. Using wavelet analysis of sunspot area and number during the north-dominated cycles (19–20), we obtained the periodicity of 160–165 days in the stronger northern hemisphere and 180–190 days in the weaker southern hemisphere. On the other hand, south-dominated cycles (21–23) display the periodicity of 155–160 days in the stronger southern hemisphere and 175–188 days in the weaker northern hemisphere. Therefore, the Rieger-type periodicity has the north–south asymmetry in sunspot area/number data during solar cycles with strong hemispheric asymmetry. We suggest that the periodicity is caused by magnetic Rossby waves in the internal dynamo layer. Using the dispersion relation of magnetic Rossby waves and observed Rieger periodicity, we estimated the magnetic field strength in the layer as 45–49 kG in more active hemispheres (north during cycles 19–20 and south during cycles 21–23) and 33–40 kG in weaker hemispheres. The estimated difference in the hemispheric field strength is around 10 kG, which provides a challenge for dynamo models. Total magnetic flux data during cycles 20–23 reveals no clear north–south asymmetry, which needs to be explained in the future.