2005学术报告

• Grad Shafranov Reconstruction Technique and Its Application 2022-11-02
• The Origin of Planetary Systems 2022-11-02
• A data driven three-dimensional magnetohydrodynamic (MHD) model for the study of the coupling between the photospherie and corona 2022-11-02
• Equatorially Trapped Middle Atmosphere Response to Global-Scale Forcing 2022-11-02
• 行星际磁场湍动的观测研究 2022-11-02
• Wave field structure in a 2- and 3-dimensionally inhomogeneous 2022-11-02
• Does the earth’s bow shock move to infinity as the magnetosonic Mach number approaching unity 2022-11-02
• Turbulence of collisionles shock front from macro to micro scales nonstationary processes (review) 2022-11-02
• The evolution of shocks near the surface of Sun during the epoch of Halloween 2003 2022-11-02
• 磁层对太阳事件的响应 2022-11-02
• Global auroral responses to solar wind dynamic pressure changes 2022-11-02
• A numerical model of the ionosphere 2022-11-02
• Peculiarities of the ionospheric response to geomagnetic storms in the East-Asian region
  1.Ionospheric effects of geomagnetic storms in different longitude sectors
  2.Variations of ionospheric parameters in quiet and weak disturbed condition 2022-11-02
• The DSP/Cluster observations of plasma sheet 2022-11-02
• Input parameters for relativistic electron flux models at geostationary orbit 2022-11-02
• The airglow during the solar - geophisical disturbances 2022-11-02
• 日冕物质抛射的行星际表现--重点研究项目进展及任务分解 2022-11-02
• CLUSTER Four Spacecraft Data Analysis Techniques --重点研究项目进展及任务分解 2022-11-02