Solar Cycle Forecasting

被引:65
作者
Hathaway, David H. [1 ]
机构
[1] NASA, MSFC, Huntsville, AL 35812 USA
关键词
Solar activity; Sunspot cycle; Solar cycle forecasting; FLUX; AMPLITUDE; DYNAMO; MINIMUM; MODELS; FIELD; SIZE;
D O I
10.1007/s11214-008-9430-4
中图分类号
P1 [天文学];
学科分类号
070403 [天体物理学];
摘要
Predicting the behavior of a solar cycle after it is well underway (2-3 years after minimum) can be done with a fair degree of skill using auto-regression and curve fitting techniques that don't require any knowledge of the physics involved. Predicting the amplitude of a solar cycle near, or before, the time of solar cycle minimum can be done using precursors such as geomagnetic activity and polar fields that do have some connection to the physics but the connections are uncertain and the precursors provide less reliable forecasts. Predictions for the amplitude of cycle 24 using these precursor techniques give drastically different values. Recently, dynamo models have been used directly with assimilated data to predict the amplitude of sunspot cycle 24 but have also given significantly different predictions. While others have questioned both the predictability of the solar cycle and the ability of current dynamo models to provide predictions, it is clear that cycle 24 will help to discriminate between some opposing dynamo models.
引用
收藏
页码:401 / 412
页数:12
相关论文
共 35 条
[1]
The predicted size of cycle 23 based on the inferred three-cycle quasi-periodicity of the planetary index Ap [J].
Ahluwalia, HS .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1998, 103 (A6) :12103-12109
[2]
THE TOPOLOGY OF THE SUNS MAGNETIC FIELD AND THE 22-YEAR CYCLE [J].
BABCOCK, HW .
ASTROPHYSICAL JOURNAL, 1961, 133 (02) :572-&
[3]
WHAT DETERMINES SUNSPOT MAXIMUM [J].
BROWN, GM .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1976, 174 (01) :185-189
[4]
On predicting the solar cycle using mean-field models [J].
Bushby, Paul J. ;
Tobias, Steven M. .
ASTROPHYSICAL JOURNAL, 2007, 661 (02) :1289-1296
[5]
Solar cycle prediction using precursors and flux transport models [J].
Cameron, R. ;
Schuessler, M. .
ASTROPHYSICAL JOURNAL, 2007, 659 (01) :801-811
[6]
Predicting solar cycle 24 with a solar dynamo model [J].
Choudhuri, Arnab Rai ;
Chatterjee, Piyali ;
Jiang, Jie .
PHYSICAL REVIEW LETTERS, 2007, 98 (13)
[7]
Predicting the strength of solar cycle 24 using a flux-transport dynamo-based tool [J].
Dikpati, M ;
de Toma, G ;
Gilman, PA .
GEOPHYSICAL RESEARCH LETTERS, 2006, 33 (05)
[8]
A Babcock-Leighton flux transport dynamo with solar-like differential rotation [J].
Dikpati, M ;
Charbonneau, P .
ASTROPHYSICAL JOURNAL, 1999, 518 (01) :508-520
[9]
Polar flux, cross-equatorial flux, and dynamo-generated tachocline toroidal flux as predictors of solar cycles [J].
Dikpati, Mausumi ;
de Toma, Giuliana ;
Gilman, Peter A. .
ASTROPHYSICAL JOURNAL, 2008, 675 (01) :920-930
[10]
FITTING THE SUNSPOT CYCLES 10-21 BY A MODIFIED F-DISTRIBUTION DENSITY-FUNCTION [J].
ELLING, W ;
SCHWENTEK, H .
SOLAR PHYSICS, 1992, 137 (01) :155-165