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20162025
most citedWill Solar Cycles 25 and 26 Be Weaker than Cycle 24 ?

30 citations

5 papers

astro-ph.SR2025★ 1 cited

Comparison Between Cycle-to-Cycle Variations in the Coefficient of Joy's Law and Covariance of Rotation Residuals and Meridional Motions of Sunspot Groups

J. Javaraiah

The tilts of bipolar magnetic regions are believed to be caused by the action of Coriolis force on rising magnetic flux tubes. Here we analysed the combined Greenwich and Debrecen…

astro-ph.SR2020★ 28 cited

Solar-Cycle Characteristics in Kodaikanal Sunspot Area: North--South Asymmetry, Phase Distribution and Gnevyshev Gap

B. Ravindra, Partha Chowdhury, J. Javaraiah

The solar activity is asymmetric in both hemispheres in almost all cycles. This asymmetry is observed both in cycle amplitude and period. We have used about 90~years of sunspot-are…

astro-ph.SR2019★ 16 cited

North--South Asymmetry in Solar Activity and Solar Cycle Prediction, IV: Prediction for Lengths of Upcoming Solar Cycles

J. Javaraiah

We analyzed the daily sunspot-group data reported by the Greenwich Photoheliographic Results (GPR) during the period 1874-1976 and Debrecen Photoheliographic Data (DPD) during the…

astro-ph.SR2017★ 30 cited

Will Solar Cycles 25 and 26 Be Weaker than Cycle 24 ?

J. Javaraiah

The study of variations in solar activity is important for understanding the underlying mechanism of solar activity and for predicting the level of activity in view of the activity…

astro-ph.SR2016★ 19 cited

Short-Term Variations in the Equatorial Rotation Rate of Sunspot Groups

J. Javaraiah, L. Bertello

We have detected several periodicities in the solar equatorial rotation rate of sunspot groups in the Greenwich Photoheliographic Results (GPR) during the period 1931-1976, the Sol…