Variations of mid-term periodicities in solar activity physical phenomena

被引:52
作者
Valdes-Gahcia, J. F. [1 ]
Velasco, V. M. [1 ]
机构
[1] Univ Nacl Autonoma Mexico, Inst Geofis, Dept Invest Solares & Planetarias, Mexico City 04510, DF, Mexico
关键词
mid-term periodicities; dynamo; wavelet coherence;
D O I
10.1016/j.asr.2007.02.012
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
In this work we make an analysis of significant periodicities shown by phenomena linked to solar activity such as coronal hole area, radio emission in the 10.7 cm band and sunspots. We use the wavelet method that gives information in the frequency and time domains. Of particular interest are the mid-term periodicities (1-2 yrs). Over the whole period, coronal holes and radio variations show an important annual variation and a quasi-biannual periodicity. The increase in these variations is most important around the years of maximum solar activity. When the time series are separated in low and high frequencies, the latter are modulated by the general solar cycle. Although somewhat shifted in frequency, these periodicities might well correspond with those found in cosmic ray intensity, solar magnetic flux and other terrestrial and interplanetary phenomena as a wavelet coherence analysis of these series with the solar magnetic flux reveals. (C) 2007 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:297 / 305
页数:9
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