The evolution of shocks near the surface of Sun during the epoch of Halloween 2003

[1]  S. Wu,et al.  Flare-generated shock evolution and geomagnetic storms during the ''Halloween 2003 epoch'': 29 October to 2 November , 2005 .

[2]  S. Wu,et al.  Slow shock interactions in the heliosphere using an adaptive grid MHD model , 2005 .

[3]  Yang Liu,et al.  Numerical Magnetohydrodynamic Experiments for Testing the Physical Mechanisms of Coronal Mass Ejections Acceleration , 2004 .

[4]  S. Wu,et al.  Evolution of fast and slow shock interactions in the inner heliosphere , 2004 .

[5]  M. Dryer,et al.  Real‐time shock arrival predictions during the “Halloween 2003 epoch” , 2004 .

[6]  A. V. Bogomolov,et al.  Solar and Heliospheric Phenomena in October–November 2003: Causes and Effects , 2004 .

[7]  J. Steinberg,et al.  Extremely high speed solar wind: 29–30 October 2003 , 2004 .

[8]  K. Ogilvie,et al.  Interplanetary slow shock observed from Wind , 1996 .

[9]  S. Wu,et al.  Numerical simulation of slow shocks in the solar wind , 1996 .

[10]  S. Wu,et al.  Generation and evolution of interplanetary slow shocks , 1996 .

[11]  S. Panitchob.  An adaptive grid finite difference method for time-dependent Magnetohydrodynamic (MHD) flows and its astrogeophysical applications , 1987 .

[12]  S. Suess,et al.  An adaptive grid, unsteady model for two-dimensional magnetohydrodynamic (MHD) flow , 1987 .

[13]  Y. Whang.  Slow shocks and their transition to fast shocks in the inner solar wind , 1987 .

[14]  H. Rosenbauer,et al.  Solar wind observations associated with a slow forward shock wave at 0.31 AU , 1984 .

[15]  L. Burlaga,et al.  REVERSE AND FORWARD SLOW SHOCKS IN THE SOLAR WIND. , 1971 .

[16]  J. Chao,et al.  Observation of slow shocks in interplanetary space , 1970 .