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Periodic variation and phase analysis of grouped solar flare with sunspot activity

Periodic variation and phase analysis of grouped solar flare with sunspot activity
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摘要 Studies on the periodic variation and the phase relationship between different solar activity indicators are useful for understanding the long-term evolution of solar activity cycles.Here we report the statistical analysis of grouped solar flare(GSF) and sunspot number(SN) during the time interval from January 1965 to March 2009.We find that,(1) the significant periodicities of both GSF and SN are related to the differential rotation periodicity,the quasi-biennial oscillation(QBO),and the eleven-year Schwabe cycle(ESC),but the specific values are not absolutely identical;(2) the ESC signal of GSF lags behind that of SN with an average of 7.8 months during the considered time interval,which implies that the systematic phase delays between GSF and SN originate from the inter-solar-cycle signal.Our results may provide evidence about the storage of magnetic energy in the corona. Studies on the periodic variation and the phase relationship between different solar activity indicators are useful for understanding the long-term evolution of solar activity cycles.Here we report the statistical analysis of grouped solar flare(GSF) and sunspot number(SN) during the time interval from January 1965 to March 2009.We find that,(1) the significant periodicities of both GSF and SN are related to the differential rotation periodicity,the quasi-biennial oscillation(QBO),and the eleven-year Schwabe cycle(ESC),but the specific values are not absolutely identical;(2) the ESC signal of GSF lags behind that of SN with an average of 7.8 months during the considered time interval,which implies that the systematic phase delays between GSF and SN originate from the inter-solar-cycle signal.Our results may provide evidence about the storage of magnetic energy in the corona.
出处 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2020年第2期75-84,共10页 天文和天体物理学研究(英文版)
基金 supported by the National Key Research and Development Program of China(2018YFA0404603) the Joint Research Fund in Astronomy(Nos.U1831204,U1931141 and U1631129)under cooperative agreement between the National Natural Science Foundation of China(NSFC)and the Chinese Academy of Sciences(CAS) the NSFC(11903009) the Yunnan Key Research and Development Program(2018IA054) the open research program of the CAS Key Laboratory of Solar Activity(KLSA201807) the major scientific research project of Guangdong regular institutions of higher learning(2017KZDXM062)
关键词 Sun:sunspots Sun:flares Sun:activity Sun:magnetic fields Sun:sunspots Sun:flares Sun:activity Sun:magnetic fields
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