Solar magnetic field structure and evolution; solar activity prediction

 
Topology of Magnetic Field and Coronal Heating in Solar Active Regions--II. The Role of Quasi-Separatrix Layers  Wang, H. N., Yan, Y. H., Sakurai, T. , Zhang, M., 2000,  Solar Phys. , 197,263-273
Topology of Magnetic Field and Coronal Heating in Solar Active Regions  Wang, H. N., Yan, Y. H., Sakurai, T. ,  2001, Solar Phys. , 201,323-336
Solar flare prediction and magnetic field evolution in solar active region  Wang, H. N.; Zhang, G. Q.; Zhu, C. L.; Sun, J. L.,  2002, Highlights of Astronomy, 12, 396-397
Long-term behavior of active longitudes for solar X-ray flares   Zhang, L. Y., Wang, H. N., Du, Z. L., Cui, Y. M., He, H., 2007,  A&A, 471(2), 711-716
Prediction of solar active longitudes   Zhang, L. Y., Wang, H. N., Du, Z. L.,  , A&A, 2008,  484(2), 523-527
Nonlinear force-free coronal magnetic field extrapolation scheme based on the direct boundary integral formulation  He, H.,  Wang, H. N.,  , 2008, JGR,  113, A5
Solar flare forecasting model supported with artificial neural network techniques  Wang, H. N., Cui, Y. M., Li, R.; Zhang, L. Y., Han, H.,  2008,  AdSpR, 42, 1464
A logistic model for magnetic energy storage in solar active regions  Wang, H. N., Cui, Y. M., He, H.,  2009, RAA, 9(6), 687-693
Study of the Poynting Flux in Active Region 10930 Using Data-driven Magnetohydrodynamic Simulation Fan, Y. L.; Wang, H. N.; He, H.; Zhu, X. S., ，2011,  ApJ， 737，39-48
What is solar electromagnetic  storm  Wang, H. N.; Ai, G. X.; Wang, J. X., 2012, SpWea. 10,  S09003