THE SUN IS OBSERVED TO BE A TORSIONAL OSCILLATOR WITH A PERIOD OF 11 YEARS

被引：431

作者：

HOWARD, R

LABONTE, BJ

机构：

来源：

ASTROPHYSICAL JOURNAL | 1980年 / 239卷 / 01期

关键词：

D O I：

10.1086/183286

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：L33 / L36

页数：4

相关论文

共 13 条

[1] IS THERE A CHRONOMETER HIDDEN DEEP IN SUN
DICKE, RH
[J]. NATURE, 1978, 276 (5689) : 676 - 680
[2] DOPPLER MEASUREMENT WITH LOW SCATTERED-LIGHT OF THE HIGHER ROTATION RATE OF SUNSPOT MAGNETIC-FIELDS AT THE PHOTOSPHERE
FOUKAL, P
[J]. ASTROPHYSICAL JOURNAL, 1979, 234 (02) : 716 - 722
[3] MOUNT WILSON SOLAR MAGNETOGRAPH - SCANNING AND DATA SYSTEM
HOWARD, R
[J]. SOLAR PHYSICS, 1976, 48 (02) : 411 - 416
[4] SPECTROSCOPIC DETERMINATIONS OF SOLAR ROTATION
HOWARD, R
HARVEY, J
[J]. SOLAR PHYSICS, 1970, 12 (01) : 23 - &
[5] POSSIBLE VARIATION OF SOLAR ROTATION WITH ACTIVITY CYCLE
HOWARD, R
[J]. ASTROPHYSICAL JOURNAL, 1976, 210 (03) : L159 - L161
[6] STUDIES OF SOLAR MAGNETIC-FIELDS .4. EFFECTS OF ANGULAR RESOLUTION
HOWARD, R
[J]. SOLAR PHYSICS, 1976, 47 (02) : 575 - 580
[7] HOWARD R, SOLAR PHYS
[8] HOWARD R, 1980, AP J, V239
[9] HOWARD R, 1974, SOL PHYS, V38, P283
[10] SOLAR ROTATION, 1966-1978
LIVINGSTON, W
DUVALL, TL
[J]. SOLAR PHYSICS, 1979, 61 (02) : 219 - 231