Solar oscillations as they are seen from minimum to maximum of solar activity

被引：0
|
作者：
Gavryusev, V [1 ]
Gavryuseva, E [1 ]
机构：
[1] CNR, CAISMI, I-50125 Florence, Italy
来源：
PROCEEDINGS OF THE SOHO 10/GONG 2000 WORKSHOP ON HELIO- AND ASTEROSEISMOLOGY AT THE DAWN OF THE MILLENNIUM | 2001年 / 464卷
关键词：
solar oscillations; helioseismology; excitation; low degree;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The GONG time series, 1692 days long, is used for the evaluation of the low-l (l = 0 - 8) p-mode parameters. The set of the mode frequencies, the most comprehensive up to date in radial orders n, is presented. The variations of mode profiles with time are discussed.
引用
收藏
页码：57 / 62
页数：6
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