2017
DOI: 10.1093/mnras/stx134
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22-year cycle of differential rotation of the solar corona and the rule by Gnevyshev–Ohl

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Cited by 13 publications
(18 citation statements)
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“…This is most probably due to the errors, which are more pronounced at the beginning of the dataset where the amount of available data in years near minima is low. Badalyan and Obridko (2017) examined the 22-year cycle of differential rotation and the rule of Genevyshev-Ohl by using the green coronal line brightness data from 1943 onward and obtained a result consistent with inverse correlation of both differential-rotation parameters and activity (see Figures 3 and 4 in Badalyan and Obridko, 2017). Their finding of larger increases of equatorial rotation velocity between even and odd cycle than between odd and even is not visible in our data (see Figure 1).…”
Section: Discussionsupporting
confidence: 67%
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“…This is most probably due to the errors, which are more pronounced at the beginning of the dataset where the amount of available data in years near minima is low. Badalyan and Obridko (2017) examined the 22-year cycle of differential rotation and the rule of Genevyshev-Ohl by using the green coronal line brightness data from 1943 onward and obtained a result consistent with inverse correlation of both differential-rotation parameters and activity (see Figures 3 and 4 in Badalyan and Obridko, 2017). Their finding of larger increases of equatorial rotation velocity between even and odd cycle than between odd and even is not visible in our data (see Figure 1).…”
Section: Discussionsupporting
confidence: 67%
“…This is not so clear for the differential-rotation parameter B where no secular changes were found. The larger average rotation velocities in minimum than in other phases of cycle, i.e., inverse correlation between solar equatorial-rotation rate and activity, was found by many authors using different methods and data (Lustig, 1983;Gilman and Howard, 1984;Balthasar, Vazquez, and Wöhl, 1986;Gupta, Sivaraman, and Howard, 1999;Zuccarello and Zappalá, 2003;Brajša, Ruždjak, and Wöhl, 2006;Jurdana-Šepić et al, 2011;Li et al, 2014;Badalyan and Obridko, 2017). Brun (2004) numerically modelled the interaction of convection and rotation with magnetic field in deep spherical shells and found that the increase of magnetic field would result in the reduction of differential rotation.…”
Section: Discussionmentioning
confidence: 95%
“…That is to say, the total rotation of the solar corona could be described as a superposition of two rotation modes: the fast mode near the equator is around 27 days, and the slow mode exceeds 30 days (Badalyan 2010). Using the same but longer database, Badalyan & Obridko (2017) investigated the time variation of the differential rotation parameters of the solar corona, and found that the equatorial rotation rate of the corona increases in the epochs of minimum between the even and odd cycles and arrives at its minimum values between the odd and even cycles. They suggested that the 22-year cycle of differential rotation pattern could be used to explain the effect by the Gnevyshev-Ohl rule.…”
Section: Introductionmentioning
confidence: 99%
“…The correlation coefficient for the curves on the right panel in the range of the periods from 50 to 250 months is 0.94. On both periodograms, the 11-yr period is weakly pronounced; however, one can clearly identify a quasi-period of 12 yr. Figure 4 represents spectral variation diagrams (SVD) for the asymmetry A (top) and the asymmetry sign sgn A (bottom) (SVD construction method is described in Badalyan et al 2005;Badalyan & Obridko 2009, 2011. A 132-month moving window was applied for calculations with a shift of 12 months.…”
Section: Basic Properties Of North-south Asymmetry Signmentioning
confidence: 99%
“…From the above it is clear that it makes sense to examine separately the asymmetry sign and its absolute value (Obridko & Badalyan 2009). The problem under discussion is formulated in Sect.…”
Section: Introductionmentioning
confidence: 99%