THINNING OF THE SUN'S MAGNETIC LAYER: THE PECULIAR SOLAR MINIMUM COULD HAVE BEEN PREDICTED

被引:48
|
作者
Basu, Sarbani [1 ]
Broomhall, Anne-Marie [2 ]
Chaplin, William J. [2 ]
Elsworth, Yvonne [2 ]
机构
[1] Yale Univ, Dept Astron, New Haven, CT 06520 USA
[2] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
来源
ASTROPHYSICAL JOURNAL | 2012年 / 758卷 / 01期
关键词
Sun: activity; Sun: oscillations; RING-DIAGRAM ANALYSIS; OSCILLATION FREQUENCIES; MODE FREQUENCIES; CONVECTION ZONE; ACTIVE REGIONS; CYCLE; 23; BISON;
D O I
10.1088/0004-637X/758/1/43
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The solar magnetic activity cycle causes changes in the Sun on timescales that are equivalent to human lifetimes. The minimum solar activity that preceded the current solar cycle (cycle 24) was deeper and quieter than any other recent minimum. Using data from the Birmingham Solar Oscillations Network (BiSON), we show that the structure of the solar sub-surface layers during the descending phase of the preceding cycle (cycle 23) was very different from that during cycle 22. This leads us to believe that a detailed examination of the data would have led to the prediction that the cycle 24 minimum would be out of the ordinary. The behavior of the oscillation frequencies allows us to infer that changes in the Sun that affected the oscillation frequencies in cycle 23 were localized mainly to layers above about 0.996 R-circle dot, depths shallower than about 3000 km. In cycle 22, on the other hand, the changes must have also occurred in the deeper-lying layers.
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页数:6
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