Xudong Sun

Ph.D. Candidate, Physics Department, Stanford University
Research Assistant, W.W. Hansen Experimental Physics Laboratory, Stanford University
Email: xudongs@stanford.edu

Evolution of Magnetic Field and Energy in a Major Eruptive Active Region Based on SDO/HMI Observation (Sun, X., Hoeksema, J. T., Liu, Y., Wiegelmann, T., Hayashi, K., Chen, Q., Thalmann, J., 2012, ApJ, accepted. pdf)
A New Method for Polar Field Interpolation (Sun, X., Liu, Y., Hoeksema, J. T., Hayashi, K., Zhao, X., 2011, Solar Physics, 270, 9. abstract pdf)
Coronal Field Opens at Lower Height During the Solar Cycles 22 and 23 Minimum Periods: IMF Comparison Suggests the Source Surface Should Be Lowered (Lee, C. O., Luhmann, J. G., Hoeksema, J. T., Sun, X., Arge, C. N., de Pater, I., 2011, Solar Physics, 269, 367. abstract reprint)
Earth's Bow Shock and Its Interaction with Interplanetary Shocks (Hu, Y. and Sun, X., 2005, Chinese J. Geophys. pdf)

Evolution of Magnetic Field and Energy in a Major Eruptive Active Region Observed by SDO/HMI (AGU 2011 poster)
Evolution of Magnetic Field and Energy in a Major Eruptive Active Region Observed by SDO/HMI (SDO3 Workshop presentation)
Evolution of Magnetic Field in AR11158 from SDO/HMI (SDO1 Workshop presentation)
First Result of Field Extrapolation Based on HMI Vector Magnetic Data (AGU 2010 poster)
HMI Global and Local Magnetic Modeling Pipeline (SPD 2010 poster)
A New Source Surface Radius in Potential Field Modeling During the Current Weak Solar Minimum? (AGU 2009 poster)
Spatial Structures of Polar Magnetic Field During the Last Solar Cycle (SPD 2009 poster)
Polar Magnetic Fields Observed During the Last Four Solar Minima (AGU 2008 poster)