On the formation of spectral line profiles of solar p modes

被引:0
|
作者
Roxburgh, IW [1 ]
Vorontsov, SV [1 ]
机构
[1] MOSCOW PHYS EARTH INST,MOSCOW 123810,RUSSIA
关键词
waves; methods; analytical; Sun; oscillations; stars; interiors;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We address the problem of the opposite asymmetry of low-frequency p-mode line profiles observed in intensity and velocity measurements. We use a simple model to illustrate that this feature can be explained by including a contribution from the stochastic excitation velocity field to the non-resonant background in the Doppler measurements.
引用
收藏
页码:L33 / L36
页数:4
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