221. Magnetic Reconnection: General Mechanism of the Whistler-mode Waves Revealed
For those of you who are not quite familiar with the concept of magnetic reconnection, it is a physical process in highly conducting plasmas in which the magnetic topology is rearranged and magnetic energy is converted into kinetic energy. Two factors, the whistler-mode waves and electron temperatur
Keywords： Published time：2013-09-04 16:13 |
222. NSSC Scientists Reveal the Control Effect of Solar Wind on the Geomagnetospheric Substorm Properties
Geomagnetospheric substorm is one of the major disturbances occurred in Earth’s magnetosphere, lasting from a period of 1 to 3 hours in most cases. As one of the most important energy input, coupling and dissipation process in geospace, it can cause the interruption of radio communication in high l
Keywords： Published time：2013-08-21 15:47 |
223. NSSC Scientists Visited Space Research Institute, the Austrian Academy of Sciences
From Jun.24 to Jun. 29, 2013, upon the invitation of Dr. Werner Magnes, Dr. WANG Jindong, Dr. ZHOU Bin and Mr. CHENG Bingjun from the Lab of Solar System Exploration, National Space Science Center (NSSC), paid a six-day visit to the Space Research Institute (Institut für Weltraumforschung, IWF), th
Keywords： Published time：2013-07-15 07:48 |
224. Scientists Performed a 3D MHD Simulation of a Realistic CME Initiation Process
Manifested as brilliant observational forms such as flares, filament eruptions and coronal mass ejections (CMEs), solar eruptions, as major drivers of space weather, have a dark side. From time to time, billions of tonnes of ionized gas, or plasma are expulsed from the solar atmosphere at millions o
Keywords： Published time：2013-07-05 08:20 |
225. NSSC Scientists Unraveled the Multiple Small-scale Plasmoid Structure in the Magnetotail
Recently, with data from European Space Agency (ESA)’s Cluster spacecraft, SIGMA team under State Key Laboratory of Space Weather, National Space Science Center (NSSC), have made the first direct observations of multiple small-scale plasmoids during a substorm. Using a magnetohydrodynamic model,
Keywords： Published time：2013-06-27 15:38 |
226. New Observations of MLT Mean Wind and Tides Achieved
In recent decades, dynamics of the Mesosphere and Lower Thermosphere (MLT) have attracted great interests among near-space scientists and have been the subject of many experimental and theoretical investigations.
A research team at Lab of Near-Space Environment Research, National Space Science Cente
Keywords： Published time：2013-06-09 08:54 |
227. NSSC Researcher Attends Workshop on “GNSS Data Application to Low Latitude Ionospheric Research” in Italy
A Workshop on GNSS Data Application to Low Latitude Ionospheric Research, co-organized by Abdus Salam International Centre for Theoretical Physics (ICTP) and Boston College (BC) of the United States, was held from May 6 to May 17, 2013, in Trieste, Italy.
Dr. Bai Weihua from National Space Science
Keywords： Published time：2013-06-04 15:24 |
228. Solar Storm Sun-to-Earth Propagation: A General Picture Discovered
True beauty lies in the sky or in space scientists’ eyes, in the vast and mysterious space with its order, extent and darkness. They explode with immense power in the solar atmosphere and are hurled out from the Sun at millions of kilometers per hour. They light up brilliant auroras in the mid-lati
Keywords： Published time：2013-05-31 07:56 |
229. Could the Collision of CMEs in the Heliosphere be Super-elastic?
Recently, space science scientists from National Space Science Center (NSSC) and University of Science and Technology in China (USTC) analyzed the energy transformation between two Coronal Mass Ejections (CMEs) after their collision based on three-dimensional (3D) numerical simulation. It is the fir
Keywords： Published time：2013-05-22 07:41 |
230. Towards a Bettering Understanding of the Moon-Solar Wind Interaction
A research team at Lab of Solar System Exploration, National Space Science Center (NSSC) has recently presented a three-dimensional magnetohydrodynamic (MHD) simulation of the lunar wake to further our understanding of the Moon-solar wind interaction.
By establishing a 3D MHD model with high spatia
Keywords： Published time：2013-05-20 14:19 |
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