Observation of hysteresis between solar activity indicators andp-mode frequency shifts for solar cycle 22

被引:0
作者
S. C. Tripathy
Brajesh Kumar
Kiran Jain
A. Bhatnagar
机构
[1] Physical Research Laboratory,Udaipur Solar Observatory
来源
Journal of Astrophysics and Astronomy | 2000年 / 21卷
关键词
Sun: oscillations, activity;
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摘要
Using intermediate degreep-mode frequency data sets for solar cycle 22, we find that the frequency shifts and magnetic activity indicators show a “hysteresis” phenomenon. It is observed that the magnetic indices follow different paths for the ascending and descending phases of the solar cycle while for radiative indices, the separation between the paths are well within the error limits.
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页码:357 / 360
页数:3
相关论文
共 13 条
[1]  
Bachmann K. T.(1993)undefined Astrophys. J. 411 L45-L45
[2]  
Brown T. M.(1999)undefined Astrophys. J. 521 885-885
[3]  
Bhatnagar A.(1998)undefined Astr. Astrophys. 329 1119-1119
[4]  
Jain Kiran(1991)undefined Astrophys. J. 373 L81-L81
[5]  
Tripathy S. C.(undefined)undefined undefined undefined undefined-undefined
[6]  
Jiménez-Reyes S. J.(undefined)undefined undefined undefined undefined-undefined
[7]  
Regulo C(undefined)undefined undefined undefined undefined-undefined
[8]  
Palleé P. L.(undefined)undefined undefined undefined undefined-undefined
[9]  
Roca Cortés(undefined)undefined undefined undefined undefined-undefined
[10]  
Woodard M. F.(undefined)undefined undefined undefined undefined-undefined