2 Zhao P, Zhou X J, Liu G. Decadal-centennial-scale change in Asian-Pacific summer thermal contrast and solar activity. Chin Sci Bull, 2011, 56: 3012-3018
[3]
3 Wu J Y, Shao X H, Kong X G, et al. Imprint of solar activity on Nanjing stalagmite annual layer thickness sequence during the Last Glacial Maximum. Chin Sci Bull, 2006, 51: 441-447
[4]
4 Liao D H, Liao X H. New evidence for possible impact of solar activity on long-term fluctuation of the earth rotation. Chin Sci Bull, 2001, 46: 905-908
25 Gallagher P T, Moon Y, Wang H M. Active-region monitoring and flare forecasting I. Data processing and first results. Solar Phys, 2002, 209: 171-183
[19]
26 Abramenko V, Yurchyshyn V, Wang H, et al. Scaling behavior of structure functions of the longitudinal magnetic field in active regions on the sun. Astrophys J, 2002, 577: 487-495
[20]
30 Wheatland M. A test to confirm the source of energy for solar flares. Pub Astron Soc Austr, 2001, 18: 351-354
[21]
33 Leka K D, Barnes G. Photospheric magnetic field properties of flaring versus flare-quiet active regions. II. Discriminant analysis. Astrophys J, 2003, 585: 1296-1306
[22]
34 Leka K D, Branes G. Photospheric magnetic field properties of flaring versus flare-quiet active regions. IV. A statistically significant sample. Astrophys J, 2007, 656: 1173-1186
[23]
37 Xie W B, Wang H M, Jing J, et al. The correlation between expansion speed and magnetic field in solar flare ribbons. Sci China Ser G- Phys Mech Astron, 2009, 52: 1754-1759
[24]
38 Cui Y M, Li R, Zhang L Y, et al. Correlation between solar flare productivity and photospheric magnetic field properties. 1. Maximum horizontal gradient, length of neutral line, number of singular points. Solar Phys, 2006, 237: 45-59
41 McAteer R T, Gallagher P T, Ireland J. Statistics of active region complexity: A large-scale fracta dimension survey. Astrophys J, 2005, 631: 628-635
[27]
44 Aschwanden M J, Aschwanden P D. Solar flare geometries. II. The volume fractal dimension. Astrophys J, 2008, 674: 544-553
[28]
48 Yu Z G, Anh V, Eastes R, et al. Multifractal analysis of flare indices and their horizontal visibility graphs. Nonlin Proc Geophys, 2012, 19: 657-665
[29]
49 Wheatland M S. A bayesian approach to solar flare prediction. Astrophys J, 2004, 609: 1134-1139
[30]
50 Wheatland M. A statistical solar flare forecast method. Space Weath, 2005, 3: S07003
[31]
51 Huang X, Yu D, Hu Q. Short-term solar flare prediction using predictor teams. Solar Phys, 2010, 263: 175-184
[32]
52 Giovanelli R G. The relations between eruptions and sunspots. Astrophys J, 1939, 89: 2555-567
[33]
53 Drake J. Characteristics of soft solar X-ray bursts. Solar Phys, 1971, 16: 152-185
[34]
56 Bornmann P, Shaw D. Flare rates and the McIntosh active-region classifications. Solar Phys, 1994, 150: 127-146
[35]
57 Bartkowiak A, Jakimiec M. Distance-based regression in prediction of solar flare activity. Questiio, 1994, 18: 7-12
[36]
58 Zhang G Q, Wang J L. A new scheme used for the short-term prediction of X-xary flares. Progr Geophys, 1994, 9: 54-58
[37]
59 Zhu C L, Wang J L. Verification of short-term prediction of solar X-ray bursts for the maximum phase (2000-2001) of solar cycle 23. Chin J Astron Astrophys, 2003, 3: 563-568
[38]
62 Baena M, Morales R. The influence of active region information on the prediction of solar flares: An empirical model using data mining. Annales Geophys, 2005, 3129-3138
[39]
63 Song H, Tan C, Jing J, et al. Statistical assessment of photospheric magnetic features in imminent solar flare predictions. Solar Phys, 2008, 254: 101-125
[40]
64 Yuan Y, Shih F Y, Jing J, et al. Automated flare forecasting using a statistical learning technique. Res Astron Astrophys, 2010, 10: 785-796
[41]
65 Ahmed O W, Qahwaji R, Colak T, et al. Solar flare prediction using advanced feature extraction, machine learning, and feature selection. Solar Phys, 2013, 283: 157-175
[42]
66 Li R, He H, Cui Y M, et al. Support vector machine combined with K-nearest neighbors for solar flare forecast. Chin J Astron Astrophys, 2007, 7: 441-447
[43]
68 Yu D R, Huang X, Wang H N, et al. Short-term solar flare prediction using a sequential supervised learning method. Solar Phys, 2009, 255: 91-105
[44]
69 Yu D R, Huang X, Wang H N, et al. Short-term solar flare prediction using multi-resolution predictors. Astrophys J, 2010, 709: 321-326
[45]
70 Yu D, Huang X, Wang H N, et al. Short-term solar flare level prediction using a bayesian network approach. Astrophys J, 2010, 710: 869-877
[46]
71 Huang X, Wang H N, Dai X H. Influences of misprediction costs on solar flare prediction. Sci China-Phys Mech Astron, 2012, 55: 1956-1962
[47]
81 Bak P, Tang C, Wiesenfeld K. Self organized criticality: An explanation of 1/f noise. Phys Rev Lett, 1987, 59: 381-384
27 Komm R, Hill F. Solar flares and solar subphotospheric vorticity. J Geophys Res Space Phys, 2009, 114: A06105
[57]
28 Hagyard M. The significance of vector magnetic field measurements. Soc Astron Ital, 1990, 61: 337-357
[58]
29 Schmieder B, Hagyard M, Ai G, et al. Relationship between magnetic field evolution and flaring sites in AR 6659 in June 1991. Solar Phys, 1994, 150: 199-219
32 Leka K D, Barnes G. Photospheric magnetic field properties of flaring versus flare-quiet active regions. I. Data, general approach, and sample results. Astrophys J, 2003, 595: 1277-1295
[61]
35 Georgoulis M K, Rust D M. Quantitative forecasting of major solar flares. Astrophys J, 2007, 661: L109-L112
[62]
36 Barnes G, Leka K D. Evaluating the preformance of solar flare forecasting methods. Astrophys J, 2008, 688: L107-L110
[63]
39 Cui Y M, Li R, He H, et al. Correlation between solar flare productivity and photospheric magnetic field properties. II Magnetic gradient and magnetic Shear. Solar Phys, 2007, 242: 1-8
[64]
42 Karakatsanis L P, Pavlos G P. SOC and chaos into the solar activity. Nonlin Phenom Compl System, 2008, 11: 280-284
[65]
43 Aschwanden M J, Aschwanden P D. Solar flare geometries. I. The area fractal dimension. Astrophys J, 2008, 674: 530-543
[66]
45 Meunier N. Complexity of magnetic structures: Flares and cycle phase dependence. Astron Astrophys, 2004, 420: 333-342
[67]
46 Lawrence J K, Ruzmaikin A A, Candavid A C. Multifractal measure of the solar magnetic field. Astrophys J, 1993, 417: 805-811
[68]
47 Conlon P A, Gallagher P T, McAteer R T J, et al. Multifractal properties of evolving active regions. Solar Phys, 2008, 248: 297-309
[69]
54 Aschwanden M, Dennis B, Benz A. Logistic avalanche processes, elementary time structures, and frequency distributions in solar flares. Astrophys J, 1998, 497: 972-993
[70]
55 Bai T. Variability of the occurrence frequency of solar flares as a function of peak hard X-ray rate. Astrophys J, 1993, 404: 805-809
[71]
60 Bradshaw G, Fozzard R, Ceci L. A connectionist expert system that actually works. Adv Neu Inform Proc Sys, 1989, 1: 248-255
[72]
61 Qahwaji R, Colak T. Automatic short-term solar flare prediction using machine learning and sunspot associations. Solar phys, 2007, 241: 195-211
[73]
67 Wang H N, Cui Y M, Li R, et al. Solar flare forecasting model supported with artificial neural network techniques. Adv Space Res, 2007, 42: 1464-1468
[74]
72 Li R, Wang H N, Huang X, et al. Solar flare forecasting using learning vector quantity and unsupervised clustering techniques. Sci China-Phy Mech Astron, 2011, 54: 1367-1554
74 Gao P X, Li K J, Li Q X. Latitude migration of solar activity at high latitudes. Chin Sci Bull, 2008, 53: 8-11
[77]
75 Huang X, Zhang L Y, Wang H N. Improving the performance of solar flare prediction using active longitudes information. Astron Astrophys, 2012, 549: A127
[78]
76 Huang X, Wang H N. Solar flare prediction using highly stressed longitudinal magnetic field parameters. Res Astron Astrophys, 2013, 13: 351-358
[79]
77 马建文. 数据同化算法研发与是实验. 北京: 科学出版社, 2013
[80]
78 Bélanger E, Vincent A, Charbonneau P. Predicting solar flares by data assimilation in avalanche models. I. Model design and validation. Solar Phys, 2007, 245: 141-165
[81]
79 Lu E D, Hamilton R J. Avalanches and the distribution of solar flares. Astrophys J, 1991, 380: L89-L92
[82]
80 Li R, Zhu J. Solar flare forecasting based on sequential sunspot data. Res Astron Astrophys, 2013, 9: 1118-1126