Supported by the National Natural Science Foundation of China(40921063,40890162,41074122);the Specialized Research Fund for State Key Laboratories
The scientific objective of solar corona and interplanetary research is the understanding of the various phenomena related to solar activities and their effects on the space environments of the Earth.Great progress ha...
Supported by the National Natural Science Foundation of China(40674082,40974106,40921063,40831060);the Specialized Research Fund for State Key Laboratories
The north-south component B_z of the Interplanetary Magnetic Field(IMF) and solar wind dynamic pressure P_d are generally treated as the two main factors in the solar wind that determine the geometry of the magnetosph...
supported by the National Natural Science Foundation of China(41074114,40921063,40804031);the Specialized ResearchFund for State Key Laboratories of China
To interpret density holes in the solar wind,which are nonlinear structures observed by Cluster and Double Star,we propose an electrostatic ion fluid model.We derive the Sagdeev potential from the magnetohydrodynamic(...
supported by the National Natural Science Foundation of China(40974099,40731054,40704027 and 40921063);the Specialized Research Fund for State Key Laboratories and the National Basic Research Program of China(2011CB811404)
Low frequency electromagnetic fluctuations in the vicinity of a magnetospheric substorm onset were investigated using simultaneous observations by THEMIS multiple probes in the near-Earth plasma sheet in the magnetota...
supported by the National Natural Science Foundation of China (Grant Nos. 40804037, 40890165, and 40921063);the National Important Basic Research Project of China (Grant No. 2011CB811405);the Chinese Meridian Project and the Specialized Research Fund for State Key Laboratories
In this paper, winds derived from OH Meinel 892.0 nm detection by an FPI (Fabry-Perot Interferometer) are compared with the simultaneous wind measurements from a meteor radar during April-May of 2010. The peak heigh...
supported by the National Natural Science Foundation of China (Grant Nos. 40921063, 41004063, 41074109, 40890165, and 41174127);the National Important Basic Research Project (Grant No. 2011CB811405);the China Postdoctoral Science Foundation (Grant No. 20100470506);supported in part by the Specialized Research Fund;the Open Research Program of the State Key Laboratory of Space Weather;the National Science Foundation of Unites States grant-ATM-0633418 to Miami University
Because of the importance of gravity waves (GWs) in coupling different atmospheric regions, further studies are necessary to investigate the characteristics of GW propagation in a non-isothermal atmosphere. Using a ...
supported by the National Natural Science Foundation of China (Grant Nos. 40974091, 41174135 and 40921063);the Specialized Research Fund for State Key Laboratories
Spread-F is a manifestation of ionospheric irregularities and generally takes place at nighttime. However, it can also be ob- served seldom at daytime, It is recognized that acoustic gravity waves (AGWs) play an imp...
supported by the National Natural Science Foundation of China (Grant Nos. 41074109, 40890165, 40921063, 41004063);the National Important Basic Research Project of China (Grant No. 2011-CB811405);the Specialized Research Fund for State Key Laboratories
A SpectroMeter of Atmospheric RadiaTion (SMART) was developed and installed at the Xinglong station of the National Astronomical Observatories in Hebei province, China, which was supported by the Meridian Project [1...