Prediction of the amplitude of sunspot cycle 23

被引:17
作者
Jain, R [1 ]
机构
[1] Udaipur Solar Observ, Phys Res Lab, Dept Space, Udaipur 313001, India
关键词
D O I
10.1023/A:1004973827442
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A few prediction methods have been developed using the 'precursor' techniques and are found to be successful. On the basis of geomagnetic activity aa indices during the descending phase of the preceding cycle, we have established an expression which predicts the maximum annual mean sunspot number in cycle 23 to be 166.2. This indicates that cycle 23 would be a highly active and historic cycle. The average geomagnetic activity aa index during the ascending phase of cycle 23 would be about 24.9, comparable to 22.2 and 24.8 in cycles 21 and 22, respectively. This further indicates that during the ascending phase of cycle 23 energetic two-ribbon flares will be produced so as to give rise to strong proton events.
引用
收藏
页码:431 / 437
页数:7
相关论文
共 21 条
[1]  
BOTELER DH, 1990, P SOL TERR PRED WORK, V2, P25
[2]  
BROWN GM, 1984, P MEUD SOL TERR PRED, V1, P1
[3]   GEOMAGNETIC AND SOLAR-WIND CYCLES, 1900-1975 [J].
FEYNMAN, J .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1982, 87 (NA8) :6153-6162
[4]  
JAIN R, 1987, MON NOT R ASTRON SOC, V223, P877
[5]  
JAIN R, 1997, UNPUB B ASTRON SOC I
[6]  
JOSELYN JA, 1996, COMMUNICATION
[7]   PREDICTED INTENSITY OF SOLAR MAXIMUM [J].
KANE, RP .
NATURE, 1978, 274 (5667) :139-140
[8]  
KOPECKY M, 1991, B ASTRON I CZECH, V42, P157
[9]  
KUNCHES J, 1993, P OTT SOL TERR PRED, V2, P198
[10]   A 2-COMPONENT SOLAR-CYCLE [J].
LEGRAND, JP ;
SIMON, PA .
SOLAR PHYSICS, 1991, 131 (01) :187-209