Principal components and independent component analysis of solar and space data

被引:22
作者
Cadavid, A. C. [1 ]
Lawrence, J. K. [1 ]
Ruzmaikin, A. [2 ]
机构
[1] Calif State Univ Northridge, Dept Phys & Astron, Northridge, CA 91330 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
Methods : statistical; Sun : magnetic field;
D O I
10.1007/s11207-007-9026-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Principal components analysis (PCA) and independent component analysis (ICA) are used to identify global patterns in solar and space data. PCA seeks orthogonal modes of the two-point correlation matrix constructed from a data set. It permits the identification of structures that remain coherent and correlated or that recur throughout a time series. ICA seeks for maximally independent modes and takes into account all order correlations of the data. We apply PCA to the interplanetary magnetic field polarity near 1 AU and to the 3.25R(circle dot) source-surface fields in the solar corona. The rotations of the two-sector structures of these systems vary together to high accuracy during the active interval of solar cycle 23. We then use PCA and ICA to hunt for preferred longitudes in northern hemisphere Carrington maps of magnetic fields.
引用
收藏
页码:247 / 261
页数:15
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