Title of article
Phase asynchrony between coronal index and sunspot numbers Original Research Article
Author/Authors
L.H. Deng، نويسنده , , Z.Q. Qu، نويسنده , , K.R. Wang، نويسنده , , X.B. Li، نويسنده ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2012
Pages
9
From page
1425
To page
1433
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.
Keywords
Methods: data analysis , Sun: corona – sunspots
Journal title
Advances in Space Research
Serial Year
2012
Journal title
Advances in Space Research
Record number
1134221
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