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161. AMAS Channel Specifications and T/V Calibration Results on FY-3C Satellite Revealed
    When the Microwave Humidity Sounder (MWHS) on board FY-3 (A/B) was designed in the Key Laboratory of Microwave and Remote Sensing at the National Space Science Center (NSSC), the research group perhaps hadn’t envisioned that before long, it will be optimized and replaced by its better version,
Keywords:     Published time:2015-01-20 16:18
162. NSSC Scientists Reveal the Correlation between Ionospheric Spread F and Scintillation in Low Latitude Region
    Based on observation data from the collocated ionospheric scintillation monitor and ionosonde at low latitude station, Dr. WANG Zheng and Prof. SHI Jiankui from the State Key Laboratory of Space Weather, the National Space Science Center, statistically analyzed the correlation between ionospher
Keywords:     Published time:2015-01-07 14:55
163. Probing into the Mechanism of the Unusual Long-lived Relativistic Electron Enhancement Event
 Recently, based on observations from the Space Particle Component Detectors (SPCDs) on Fengyun-1, an unusual long-lived relativistic electron enhancement event is investigated in detail?record=1&primarykeyvalue=DOCID2%3D%27134926%27&channelid=41343 by Dr. YANG Xiaochao, Prof. Zhu Guangwu, and Dr. SUN Yueqiang from the Laboratory of Space Environment Exploration
Keywords:     Published time:2015-01-07 11:32
164. First Statistical Study on K-H Wave Properties at Earth’s Magnetopause made by NSSC Scientists
 Have you ever seen wind blowing over water when the instability manifests in waves on the water surface? Well, it’s similar for the Kelvin-Helmholtz (K-H) waves. To be more specific, “Kelvin-Helmholtz Instability” can be excited at the interface if there is sufficient velocity shear between the t
Keywords:     Published time:2014-12-01 17:04
165. Two Classes of High-speed Flow Found Exist in the Magnetotail Causing Different Effect of Geospace environment
 Recently, based on observations from NASA’s THEMIS mission (The Time History of Events and Macroscale Interactions during Substorms), two researchers from the State Key Laboratory of Space Weather, the National Space Science Center (NSSC), Dr. LI Hui and Prof. WANG Chi, jointly with Prof. FU Suiyan
Keywords:     Published time:2014-11-04 16:13
166. New CME/Shock Arrival Time Prediction Model Proposed by NSSC Scientists
 Solar transients, such as coronal mass ejections (CMEs) and their related interplanetary (IP) shock waves, have severe space weather effects. Therefore, predicting their evolutions in the heliosphere and arrival times at Earth is an important component of space weather predictions. Recently, a new g
Keywords:     Published time:2014-10-13 16:04
167. NSSC Scientists Reveal the Entropy Generation Mechanism across a Collisionless Shock
 Collisionless shocks are of great interest in space physics, plasma physics, and astrophysics. In the shock transition, the bulk energy of plasma is converted into thermal energy in the absence of particle collisions. The shock is also thought to be an important source of high-energy particles (e.g.
Keywords:     Published time:2014-09-16 17:35
168. NSSC Scientists Reveal the Control Effect of IMF By on the Field-aligned Current in the Magnetotail during Northward Int
 A research team composed of Dr. CHENG Zhengwei, Prof. SHI Jiankui, Prof. Dunlop M and Prof. LIU Zhenxing from the State Key Laboratory of Space Weather, the National Space Science Center (NSSC) recently breaks the deadlock and revealed the influence of the Interplanetary Magnetic Field (IMF) By comp
Keywords:     Published time:2014-08-14 14:25
169. The Distribution of Ring Current and its Magnetic Structure Revealed by NSSC Scientists
 A Magnetic storm is a temporary geomagnetic disturbance occurred in the Earth’s magnetosphere. It is the prime physical processes of the magnetospheric space weather. Ring Current (RC), an electric current carried by charged particles trapped in a planet's magnetosphere, is recognized as the key is
Keywords:     Published time:2014-08-13 16:03
170. NSSC Scientists Reveal the Control Effect of IMF on the Twisting of Magnetotail
 Known as the abrupt boundary between the planet’s magnetic field and the solar wind, magnetopause is one of the most important regions of solar wind-magnetosphere coupling. The study of its shape is not only of vital importance to space weather forecast, but also fundamental and crucial when it com
Keywords:     Published time:2014-07-11 15:51
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