supported by the National Natural Science Foundation of China(42222408,41931073);supported by the Youth Innovation Promotion Association of the Chinese Academy of Sciences(Y2021027);supported by the Key Research Program of the Institute of Geology&Geophysics,Chinese Academy of Sciences(grant IGGCAS-201904).
The dune aurora,at a scale of~30 kilometers,was reported recently using ground camera.The small-scale dune aurora occurs on the duskside and exhibits a monochromatic oscillation in the auroral emission,implying fundam...
supported by National Natural Science Foundation of China (41674155 and 41274147);Youth Innovation Promotion Association of Chinese Academy of Sciences (No.2017258);Key Research Project of Chinese Academy of Sciences:Application Research on the Scientific Data from Chang’E-3 Mission (KGZD-EW-603)
The plasmapause locations determined from the Chang'e-3(CE-3) Extreme Ultraviolet Camera(EUVC) images and the auroral boundaries determined from the Defense Meteorological Satellite Program(DMSP) Special Sensor Ultrav...
The plasmasphere is a region of relatively dense (-10-10000 cm^-3) plasma, surrounding the Earth and ex- tending to distances of about five Earth radii (RE). It is filled with large amount of cold (-1 eV) plasma...
supported by the National Natural Science Foundation of China(Grant Nos.41104109,41274166);the Specialized Research Fund for State Space Weather Key Laboratories(Grant No.201203FSK05)
A new empirical model of plasmapause location as functions of magnetic local time and geomagnetic indices has been developed based on the observations from THEMIS mission. We use the two-year data of electron density ...
the National Natural Science Foundation of China (Grant Nos. 40504017, 40636031)
The characteristic and properties of ULF waves in the plasmasphere boundary layer during two very quiet periods are present. The ULF waves were detected by Double Star TC-1 when the spacecraft passed through the plasm...