Storm-Time Strong Field-Aligned Ion Upflow in Region of the SED Plume
YUAN Zhi-Gang1,2, DENG Xiao-Hua1, WANG Jing-Fang1
1School of Electronic Information, Wuhan University, Wuhan 4300722Sate Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080
Storm-Time Strong Field-Aligned Ion Upflow in Region of the SED Plume
YUAN Zhi-Gang1,2, DENG Xiao-Hua1, WANG Jing-Fang1
1School of Electronic Information, Wuhan University, Wuhan 4300722Sate Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing 100080
摘要We report the observations from the GPS TEC and DMSP F-13 satellites showing that very strong upward field-aligned (FA) ion velocity and flux in the outer region of the storm-enhanced density (SED) occurred in the event of the geomagnetic storm on 29--31 May 2003. By a method of coordinate transformation, upward FA ion velocities in excess of 250m/s are obtained from the observations of the DMSP F-13 satellite. Further, an FA ion flux is estimated to be about 4.5i×1013ions/m2s in the dusk sector. The estimated FA ion velocity and flux provide a powerful direct proof to support the scenario that there is a strong coupling of particles between the ionosphere and plasmasphere in the region of the SED plume. In the process, FA ion flux transports from the ionosphere to the plasmasphere in the region of the SED plume. Therefore, the plume of SED in the ionosphere provides an important source to the enhanced density of O+ in the storm-time plasmasphere.
Abstract：We report the observations from the GPS TEC and DMSP F-13 satellites showing that very strong upward field-aligned (FA) ion velocity and flux in the outer region of the storm-enhanced density (SED) occurred in the event of the geomagnetic storm on 29--31 May 2003. By a method of coordinate transformation, upward FA ion velocities in excess of 250m/s are obtained from the observations of the DMSP F-13 satellite. Further, an FA ion flux is estimated to be about 4.5i×1013ions/m2s in the dusk sector. The estimated FA ion velocity and flux provide a powerful direct proof to support the scenario that there is a strong coupling of particles between the ionosphere and plasmasphere in the region of the SED plume. In the process, FA ion flux transports from the ionosphere to the plasmasphere in the region of the SED plume. Therefore, the plume of SED in the ionosphere provides an important source to the enhanced density of O+ in the storm-time plasmasphere.
YUAN Zhi-Gang;DENG Xiao-Hua;WANG Jing-Fang. Storm-Time Strong Field-Aligned Ion Upflow in Region of the SED Plume[J]. 中国物理快报, 2008, 25(7): 2721-2724.
YUAN Zhi-Gang, DENG Xiao-Hua, WANG Jing-Fang. Storm-Time Strong Field-Aligned Ion Upflow in Region of the SED Plume. Chin. Phys. Lett., 2008, 25(7): 2721-2724.
2008, Vol. 25 
