Supported by the National Natural Science Foundation of China(40374056,40536029,40574068);the International Collaboration Research Team Program of Chinese Academy of Sciences
The 16 August 1999 EUV brightenings are numerically simulated by a third-order upwind compact scheme,basing on the TRACE observation.The present simulation can give a possible explanation to its formation and evolutio...
AFOSR (Grant No. FA9550-07-1-0468);AURA Sub-Award C10569A of NSO’s Cooperative Agreement AST 0132798, and NSF (Grant No. ATM-0754378);CCW is supported by NASA grant NNX07AH85G, FENG is supported by National Natural Science Foundation of China (Grant Nos. 40536029, 40621003, 40374056 and 40574058)
In recent years remarkable advances have been made in the development of phys-ics based models of various parts of the solar-terrestrial system (see JASTP special issues, October, November 2004; February 2007). In thi...
jointly supported by the National Natural Science Foundation of China(Grant Nos.40536029,40336053 and 40374056);the International Collaboration Research Team Program of the Chinese Academy of Sciences.
Aiming at two intense shock events on October 28 and 29, 2003, this paper presents a two-step method, which combines synoptic analysis of space weather ——“observing” and quantitative prediction ——“palpating”, ...
Supported by the National Natural Science Foundation of China (40374056, 40536029, 40574068)the International Collaboration Research Team Program of the Chinese Academy of Sciences
A new numerical scheme of 3rd order Weighted Essentially Non-Oscillatory (WENO) type for 2.5D mixed GLM-MHD in Cartesian coordinates is proposed. The MHD equations are modified by combining the arguments as by Dellar ...
Supported by the National Natural Science Foundation of China (40374056, 40204010, 40536029)the International Collaboration Research Team Program of the Chinese Academy of Sciences
A three-dimensional MHD simulation is conducted to study the steady solar wind in Carrington Rotation (CR) 1935 by using the three-dimensional numerical magnetohydrodynamic (MHD) model introduced by Feng et al The num...
Supported by the National Natural Science Foundation of China(40374056,40333034);Chinese Academy of Science KZCX3-SW-217,KGCX2-SW-408,KGCX3-SYW-403
This paper summarizes the research results obtained by Chinese scientists and/or through international collaborations during 2004 to 2006.Within the context of COSPAR,the progresses in the studies of the middle and up...
Supported by the National Natural Science Foundation of China (40536029, 40336053, 40374056, 40574068) and the International Collaboration Research Team Program of the Chinese Academy of Sciences
Considerable progress for the study of solar corona physics has been achieved by China's space physics community. It involves the theoretical study of coronal process of solar active phenomena, solar wind origin, acce...
Supported by the National Natural Science Foundation of China (40374056) and The KIP Pilot Project (KZCX3-SW-144) of Chinese Academy of Sciences
This paper reviews the recent studies on the ionospheric weather and climate. As a national report prepared for COSPAR, the works concerned here are limited to those made by Chinese scientists during 2004-2006. The ma...