Principal component analysis of polar cap convection

被引:11
|
作者
Kim, H. -J. [1 ]
Lyons, L. R. [1 ]
Ruohoniemi, J. M. [2 ]
Frissell, N. A. [2 ]
Baker, J. B. [2 ]
机构
[1] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA 90095 USA
[2] Virginia Polytech & State Univ, Bradley Dept Elect & Comp Engn, Blacksburg, VA USA
基金
美国国家科学基金会;
关键词
FIELD;
D O I
10.1029/2012GL052083
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We apply a statistical technique called Principal Component Analysis (PCA) for examining underlying patterns of polar cap convection and illustrate potential applications of the PCA-based dimension reduction. Two principal components are identified: the first mode (PC1) is related to "uniform variation" of the flow speed at all MLTs, and is primarily governed by IMF Bz. The second mode (PC2) is related to "dawn-dusk asymmetry", and is predominantly driven by IMF By. PCA gives the relative variance contribution of the two modes: PC1 giving similar to 42% of the total variance and PC2 similar to 17% of the total variance, which is about 40% of that from PC1. Due to the orthogonality of the principal components, the degree of dawn-dusk asymmetry can be represented by P-2, where P-2 is a component value when the observed data are projected along PC2. We identified P2 as proportional to IMF By, which leads to stronger dawn flows for By > 0 and stronger dusk flows for By < 0. The same primary modes are found regardless of the IMF orientation, implying that they are intrinsic properties of the average polar cap convection. Citation: Kim, H.-J., L. R. Lyons, J. M. Ruohoniemi, N. A. Frissell, and J. B. Baker (2012), Principal component analysis of polar cap convection, Geophys. Res. Lett., 39, L11105, doi: 10.1029/2012GL052083.
引用
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页数:5
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