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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.
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页码:L33 / L36
页数:4
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