Phase asynchrony between coronal index and sunspot numbers |
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Authors: | L.H. Deng Z.Q. Qu K.R. Wang X.B. Li |
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Affiliation: | 1. National Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, P.O. Box 110, 650011 Kunming, PR China;2. Graduate School of the Chinese Academy of Sciences, ShijingShan Block, 100049 Beijing, PR China;3. North China Electric Power University, Beijing 102206, PR China |
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Abstract: | In this paper, the phase asynchrony between coronal index and sunspot numbers is investigated. It is found that, (1) the sunspot numbers begin one month earlier than coronal index, which should mathematically lead to phase asynchrony between them but with a slight effect; (2) the 11-year Schwabe cycle is the only one period with statistical significance for coronal index and sunspot numbers, and the difference between the length of the Schwabe cycle of them should also lead to phase asynchrony between them; (3) although coronal index and sunspot numbers are coherent in low-frequency components corresponding to the 11-year Schwabe cycle, they are asynchronous in phase in high-frequency components; (4) their different definitions and physical meanings may be a major reason why there is a phase asynchrony between them. |
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Keywords: | Sun: corona &ndash sunspots Methods: data analysis |
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