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

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1997年 / 292卷 / 01期

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

页码：L33 / L36

页数：4

共 6 条

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ROXBURGH IW, 1995, MON NOT R ASTRON SOC, V272, P850

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