Observational cross helicity on the solar surface

被引:0
作者
MingYu Zhao
XiaoFan Wang
HongQi Zhang
机构
[1] Chinese Academy of Sciences,Key Laboratory of Solar Activity, National Astronomical Observatory
来源
Science China Physics, Mechanics and Astronomy | 2014年 / 57卷
关键词
cross helicity; photosphere; magnetic fields; solar activity;
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中图分类号
学科分类号
摘要
We analyzed the correlation of the solar magnetograms and Dopplergrams from SOHO/MDI and SDO/HMI respectively. It is found that the full disk correlation coefficient of Dopplergrams is more than 0.80 between SOHO/MDI and SDO/HMI. The full disk correlation coefficient of magnetograms is about 0.73 and is more than 0.95 for active regions only. We also analyzed the distribution of the cross helicity (velocity-magnetic-field correlation) on the solar surface. It is found that the latitude distributions of the cross helicity based on SOHO/MDI data and SDO/HMI data have similar tendencies, and in the analysis of solar active regions the amplitude of the horizontal component of the mean cross helicity is about two times the line-of-sight one.
引用
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页码:589 / 596
页数:7
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