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国家自然科学基金(41104090)

作品数:2 被引量:4H指数:2
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Simultaneous optical and radar observations of poleward moving auroral forms under different IMF conditions被引量:2
2012年
Using high temporal resolution optical data obtained from three-wavelength all-sky imagers at Chinese Yellow River Station in the Arctic, together with the EISCAT Svalbard radar (ESR) and SuperDARN radars, we investigated the dayside pole- ward moving auroral forms (PMAFs) and the associated plasma features in the polar ionosphere under difibrent interplanetary magnetic field (1MF) conditions, between 0900 and 1010 UT on 22 December 2003. Simultaneous optical and ESR observations revealed that all PMAFs were clearly associated with pulsed particle precipitations. During northward IMF, particles can precipi- tate into lower altitudes and reach the ionospheric E-region, and there is a reverse convection cell associated with these PMAFs. This cell is one of the typical signatures of the dayside high-latitude (lobe) reconnection in the polar ionosphere. These results indicate that the PMAFs were associated with the high-latitude reconnection. During southward IMF, the PMAFs show larger lati- tudinal motion, indicating a longer mean lifetime, and the associated ionospheric features indicate that the PMAFs were generated by the dayside low-latitude reconnection.
XING ZanyangYANG HuigenHAN DeshengWU ZhensenLIU JunmingHU ZejunZHANG QingheLIU YonghuaZHANG BeichenHU Hongqiao
关键词:RECONNECTION
Dayside poleward moving auroral forms and ionospheric convection under stable interplanetary magnetic field (IMF) conditions被引量:2
2013年
Using high temporal resolution optical data obtained from three-wavelength all-sky imagers over six winters continuously at Yellow River Station (78.92°N,11.93°E) in Arctic,we statistically investigated the dependence of location of poleward moving auroral forms (PMAFs) on the interplanetary magnetic field (IMF) B z and B y components as a function of MLT and MLAT under stable IMF conditions.It is found that more PMAFs occurred in lower latitude for Bz<0 and there was less evident IMF B y-related prenoon-postnoon asymmetry for Bz<0 than for Bz>0.We found that the PMAFs were distributed over a wide range of MLT when Bz<0,which indicates that the reconnection X-line might spread like an ’S’ shape.However,during northward IMF,PMAFs were observed predominantly prenoon for IMF By>0 and postnoon for IMF By<0 associating with the effect of the high-latitude reconnection,which is largely consistent with the theoretical model of the convection flow.
XING ZanYangYANG HuiGenHAN DeShengWU ZhenSenLIU JunMingHU ZeJunZHANG QingHeHU HongQiaoLIU YongHua
关键词:RECONNECTION
Spontaneous and trigger-associated substorms compared: Electrodynamic parameters in the polar ionosphere
The precise nature of the physical mechanism leading to the substorm expansion onset and to different recoveri...
Y.Kamide
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