On the Power Distribution of Solar p MODES

被引:0
作者
H-Y. Chang
D. O. Gough
机构
[1] Samsung Aerospace Industries Ltd,
[2] Institute of Astronomy and Department of Applied Mathematics and Theoretical Physics,undefined
来源
Solar Physics | 1998年 / 181卷
关键词
Distribution Function; Energy Distribution; Idealize Model; Power Distribution; Solar Mode;
D O I
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中图分类号
学科分类号
摘要
We present a simple idealized model of stochastically forced solar oscillations, and compare the distribution function of energy, averaged over 12-hour intervals, with that of low-degree solar modes. We find that the simulated energy distribution is similar to the observations, except at extremely high energy.
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页码:251 / 263
页数:12
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共 46 条
[1]  
Antia H. M.(1986)undefined Astrophys. Space Sci. 118 169-undefined
[2]  
Chitre S. M.(1992)undefined Monthly Notices Royal Astron. Soc. 255 603-undefined
[3]  
Narasimha D.(1992)undefined Monthly Notices Royal Astron. Soc. 255 639-undefined
[4]  
Balmforth N. J.(1994)undefined Astron. Astrophys. 285 L29-undefined
[5]  
Balmforth N. J.(1995)undefined Astron. Astrophys. 311 1024-undefined
[6]  
Baudin F.(1997)undefined Monthly Notices Royal Astron. Soc. 287 51-undefined
[7]  
Gabriel A.(1982)undefined Monthly Notices Royal Astron. Soc. 198 141-undefined
[8]  
Gibert D.(1989)undefined Astrophys. J. 341 L103-undefined
[9]  
Baudin F.(1993)undefined Astrophys. J. 410 829-undefined
[10]  
Gabriel A. H.(1993)undefined Astron. Astrophys. 214 935-undefined