Anticorrelated coupling p-modes

被引：3
作者：
Roth, M [1 ]
机构：
[1] Kiepenheuer Inst Sonnenphys, D-79104 Freiburg, Germany
来源：
ASTROPHYSICAL JOURNAL | 2001年 / 559卷 / 02期
关键词：
convection; methods : data analysis; Sun : interior; Sun : oscillations;
D O I：
10.1086/322363
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Using data from the Michelson Doppler Imager and the Global Oscillation Network Group project, we demonstrate that there exists an excess of anticorrelated power variations of pairs of solar p-modes. We find a possible explanation for this behavior in the influence of poloidal velocity fields, which may lead to coupling of p-modes that results in an energy redistribution among the solar oscillations.
引用
收藏
页码：1165 / 1170
页数：6
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