作者: H. Shimazu , T. Tanaka , Mitsue Den , T. Obara
DOI: 10.1109/APRASC.2004.1422574
关键词:
摘要: Our research activity in computer simulations of the solar wind interaction with magnetosphere is reviewed. First, results global MHD simulation Earth's are shown. They provided us a new insight into field-aligned current system, structure magnetospheric convention, and substorm mechanism. Then, we applied code to real-time operation. The helps improve model by comparing accumulated data observations. Finally, hybrid an unmagnetized planet was carried out extend ion cyclotron radius scale,