Ng, C. S.
||Three-Dimensional Simulations of the Parker’s Model of Solar Coronal Heating: Lundquist Number Scaling due to Random Photospheric Footpoint Motion
||Ng, C. S.; Lin, L.; Bhattacharjee, A.
||High Lundquist Number Resistive MHD Simulations of Magnetic Reconnection: Searching for Secondary Island Formation
||Ng, C. S.; Ragunathan, S.
||Current Sheet Statistics in Three-Dimensional Simulations of Coronal Heating
||Lin, L.; Ng, C. S.; Bhattacharjee, A.
||Distribution of Nanoflares as Spatially Resolved Current Sheets in the Solar Corona
||Ng, C. S.; Lin, L.