2013学术报告

• PLASMASPHERIC DATA ASSIMILATION AND GROUND-BASED OBSERVATIONS OF THE PLASMASPHERE 2022-11-03
• Magnetosphere-ionosphere connection in 3D-force balanced magnetic field configurations driven by empirical plasma sheet pressure under different geomagnetic conditions 2022-11-03
• Ionic Charge States of Energetic Particles： A Clue to their Origin and Acceleration 2022-11-03
• Ionospheric longitudinal variations caused by geomagnetic declination 2022-11-03
• Coratating Interaction Regions and the 27-day Variation of Galactic Cosmic Rays Intensity at 1 AU during the Cycle 23/24 Solar Minimum 2022-11-03
• A METHOD OF USING CT TECHNIQUE FOR STUDYING THE GLOBAL DENSITY OF EARTH PLASMASPHERE BY ITS EUV IMAGES 2022-11-03
• ESA's Satellite Trio SWARM 2022-11-03
• Voyager： First Observations in the Interstellar Medium 2022-11-03
• What we know and don't know about solar wind measurements and interpretation 2022-11-03
• 地球环电流动力学研讨会 2022-11-03
• Analysis of Gravity Wave Parameters from GPS Radio Occultation Temperature Data and Variations of Gravity Wave Parameters during Stratospheric Sudden Warmings 2022-11-03
• Latest Radiation Belt Storm Probes （RBSP）science results 2022-11-03
• Dipolarization fronts in the Earth's magnetotail： their interactions with ions 2022-11-03
• Global MHD Simulation of the Coronal Mass Ejection on 2011 March 7： from Chromosphere to 1 AU 2022-11-03
• Magnetar Giant Flares and Precursors --- Flux Rope Eruptions with Current Sheets 2022-11-03
• Using data assimilation to estimate outer radiation belt phase space and source rate parameters 2022-11-03
• 热层中性风的垂直与水平变化 2022-11-03
• D HYBRID CODE IN MAGNETOTAIL DYNAMICS 2022-11-03
• On Earth-Affecting Coronal Mass Ejections： Observations, Theory and Numerical Simulations 2022-11-03
• Recent advances in our understanding of magnetotail bursty convection and its consequences 2022-11-03