supported by the 973 program under grant 2012CB825601;the Chinese Academy of Sciences (KZZD-EW-01-4);the National Natural Science Foundation of China (Nos.41204126,41231068,41274192,41031066 and 41374176);the Specialized Research Fund for State Key Laboratories;supported by NSFAGS1153323 and AGS1062050;support by the Youth Innovation Promotion Association of CAS (2015122)
Solar active region (AR) 11283 is a very magnetically complex region and it has produced many eruptions. However, there exists a non-eruptive filament in the plage region just next to an eruptive one in the AR, whic...
supported by the 973 program under grant 2012CB825601;the Chinese Academy of Sciences (KZZD-EW-01-4);the National Natural Science Foundation of China (41204126,41274192,41031066 and 41074122);the Specialized Research Fund for State Key Laboratories;supported by the Youth Innovation Promotion Association of CAS (2015122)
In the solar corona, the magnetic flux rope is believed to be a fundamental structure that accounts for magnetic free energy storage and solar eruptions. Up to the present, the extrapolation of the magnetic field from...
supported by the National Basic Research Program of China(Grant Nos.2012CB825601,2014CB845903,2012CB825604);the National Natural Science Foundation of China(Grant Nos.41031066,41231068,41274192,41074121,41204127,41174122);the Knowledge Innovation Program of the Chinese Academy of Sciences(Grant No.KZZD-EW-01-4);the Specialized Research Fund for State Key Laboratories
We present a newly developed global magnetohydrodynamic(MHD) model to study the responses of the Earth's magnetosphere to the solar wind. The model is established by using the space-time conservation element and solut...
Supported by the National Basic Research Program of China(2012CB825601);the National Natural Science Foundationof China(41031066,41231068,41274192,41074121,41204127);the Knowledge Innovation Program of the ChineseAcademy of Sciences(KZZD-EW-01-4);the Specialized Research Fund for State Key Laboratories
A new hybrid numerical scheme of combining an E-CUSP(Energy-Convective Upwind and Split Pressure) method for the fluid part and the Constrained Transport(CT) for the magnetic induction part is proposed.In order to avo...
supported by the National Natural Science Foundation of China(Grant Nos.41031066,41231068,41274192,41074121&41074122);the National Basic Research Program of China(Grant No.2012CB825601);the Knowledge Innovation Program of the Chinese Academy of Sciences(Grant No.KZZD-EW-01-4);the Specialized Research Fund for State Key Laboratories
High-performance computational models are required to make the real-time or faster than rea^-time numerical prediction of adverse space weather events and their influence on the geospace environment. The main objectiv...