2011学术报告

• Hot Flow Anomalies & Foreshock Cavities − Are They the Same Thing? 2022-11-03
• Dipolarization front at magnetotail: Electric field and electron acceleration 2022-11-03
• The Interaction of Mars with the Solar Wind: Induced Magnetosphere and Ionospheric Ion Outflow 2022-11-03
• 太阳风里的波动和湍流 2022-11-03
• Solar-terrestrial physics at NCAR’s high Altitude Observatory 2022-11-03
• At the base of space weather: understanding the dynamics of the solar corona 2022-11-03
• Inflow density influence of magnetic reconnection 2022-11-03
• Anomalous magnetosheath flows and distorted subsolar magnetopause for radial interplanetary magnetic field 2022-11-03
• Ubiquitous high-speed solar coronal outflows revealed by both imaging and spectroscopic observations 2022-11-03
• The Large-scale Reconnection Geometry at the Magnetopause during Northward IMF 2022-11-03
• Reconstruction of halo CMEs using elliptic cone model and the numerical space-weather prediction model 2022-11-03
• Simulated STEREO views of the Solar Wind following the CMEs of 1 August 2010 2022-11-03
• Large scale solar wind structures 2022-11-03
• Physical model of geomagnetic sudden commencement (SC) 2022-11-03
• Earthquake (M=9.0) occurred off the Pacific coast of north-east Japan on Mar 11, 2011 and ionospheric disturbances caused by it 2022-11-03
• Energy source for auroral electrons from two proposed substorm onset process 2022-11-03
• Particle and Field Signatures in the Substorm Trigger Region 2022-11-03
• GPU上的科学计算 2022-11-03
• Aic-polarized structures in the solar wind Understanding events seen by Cluster and Ulysses 2022-11-03
• Cooperative studies of the Earth’s magnetosphere 2022-11-03