[P-EM13] 太陽地球系結合過程の研究基盤形成

[PEM13-12] Combined contribution of solar illumination, solar activity, and convection to ion upflow above the polar cap

*Yu-Zhang Ma¹、Qinghe Zhang¹、Zanyang Xing¹、P. T. Jayachandran²、J. Moen³、Roderick A. Heelis⁴、Yong Wang¹ (1.Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, Shandong University, Weihai, 264209, China、2.Physics Department, University of New Brunswick, Fredericton, New Brunswick, Canada、3.Department of Physics, University of Oslo, Oslo, Norway、4.William B. Hanson Center for Space Sciences, University of Texas at Dallas, Richardson, Texas, USA)

キーワード：Ion upflow above polar cap region , upflow occurrence increases with increasing solar zenith angle , A sesosnal diffrence in upflow velocity and flux is observed for low convection speeds but not for high convection speeds

By analyzing a 5-year period (2010-2014) of DMSP plasma data, we investigated ion upflow occurrence, speed, density, and flux above the polar cap in the northern hemisphere under different solar zenith angle (SZA), solar activity (F10.7), and convection speed. Higher upflow occurrence rates in the dawn sector are associated with regions of higher convection speed, while higher upflow flux in the dusk sector is associated with higher density. The upflow occurrence increases with convection speed and solar activity, but decreases with SZA. Upflow occurrence is the lowest when the SZA>100o and the convection speeds are low. While, the upflow velocity and flux show a clear seasonal dependence with higher speed in the winter and higher flux in the summer during low convection conditions. However, they are detected for the first time to be both higher in summer during high convection conditions. These results suggest that ion upflow in the polar cap is controlled by the combination of convection, solar activity, and solar illumination.