THE VARIATION IN THE STRENGTH OF LOW-L SOLAR P-MODES - 1981-92

被引：43

作者：

ELSWORTH, Y ^{[1
]}

HOWE, R ^{[1
]}

ISAAK, GR ^{[1
]}

MCLEOD, CP ^{[1
]}

MILLER, BA ^{[1
]}

NEW, R ^{[1
]}

SPEAKE, CC ^{[1
]}

WHEELER, SJ ^{[1
]}

机构：

[1] SHEFFIELD HALLAM UNIV,SCH SCI,SHEFFIELD S1 1WB,S YORKSHIRE,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1993年 / 265卷 / 04期

关键词：

SUN; INTERIOR; OSCILLATIONS;

D O I：

10.1093/mnras/265.4.888

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The acoustic eigenmodes of the Sun are a well-recognized probe of the structure of the solar interior. We report here on a measurement of the strength of the low-l p-mode oscillations throughout a solar cycle. There is an increase of 35 +/- 5 per cent in the strength of the modes from solar maximum to solar minimum, consistent for all the l-values measured. The observations were made with the Birmingham Solar Oscillations Network ('BISON').

引用

页码：888 / 898

页数：11

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