Relative phase analyses of long-term hemispheric solar flare activity |
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| Authors: | K J Li P X Gao L S Zhan X J Shi W W Zhu |
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| Institution: | National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China;Key Laboratory of Solar Activity, National Astronomical Observatories, CAS, Beijing 100012, China;School of Graduate, CAS, Beijing, China;Jingdezhen Ceramic Institute, Jingdezhen 333001, Jiangxi, China |
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| Abstract: | Wavelet transform methods, including the continuous wavelet transform, cross-wavelet transform and wavelet coherence, have been proposed to investigate the phase synchrony of the monthly mean flare indices in the time interval 1966 January–2007 December in the solar northern and southern hemispheres, respectively. The Schwabe cycle is the only period of statistical significance, and its mean value is 10.7 yr for the monthly mean flare indices in the northern hemisphere but slightly smaller, 10.1 yr, in the southern hemisphere – this should lead to phase asynchrony between the two. Both the cross-wavelet transform and wavelet coherence analyses show asynchronous behaviour with strong phase mixing in the high-frequency components of hemispheric flare activity, and strong synchronous behaviour with coherent phase angles in the low-frequency components, corresponding to the period-scales around the Schwabe cycle. The northern flare activity should lead the southern for the low-frequency components. |
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| Keywords: | methods: data analysis Sun: activity Sun: flares |
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