JpGU-AGU Joint Meeting 2017

講演情報

[EE]Eveningポスター発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM12] [EE] Space Weather, Space Climate, VarSITI

2017年5月23日(火) 17:15 〜 18:30 ポスター会場 (国際展示場 7ホール)

[PEM12-P30] Multi-instrument observations of periodic poleward moving polar cap arcs

*Zan-Yang Xing1Qing-He Zhang1Desheng Han2Yongliang Zhang3Jun Liang4Joran Moen5Zejun Hu2P. Jayachandran6Natsuo Sato7Shunrong Zhang8Keisuke Hosokawa9Y. Wang1Yu-Zhang Ma1 (1.Shandong University、2.Research Institute of China、3.Johns Hopkins University、4.University of Calgary、5.University of Oslo、6.University of New Brunswick、7.National Institute of Polar Research、8.Massachusetts Institute of Technology、9.University of Electro-Communications)

キーワード:periodic poleward moving arcs, plasma velocity shears, magnetic reconnection

Polar cap arcs (PCAs) are one of the outstanding phenomena in the polar cap region. We examined a case of periodic poleward moving arcs observed on January 3, 2014 by dual all-sky imagers, one at the Chinese Yellow River Station (YRS) and the other at Resolute Bay (RSB), the spaced-based SSUSI imager onboard DMSP spacecraft and Resolute Bay Incoherent Scatter Radar (RISR) during quiet geomagnetic conditions. We found that some poleward moving arcs observed at RSB were repeatedly detached from the dawnside auroral oval, which is consistent with the IMF-By polarity, and some arcs observed at YRS were likely less poleward moving from the duskside auroral oval. We also observed some periodic spatial arcs by DMSP SSUSI imagers and strong plasma velocity shears around these arcs. At the same time, the precipitating particles observed in the ionosphere associated with these PCAs showed magnetospheath-like properties. Moreover, the RISR data show that the F-region plasmas above these arcs were structured, with significant E-region ionization above an intense arc. Based on these observational results, we suggest that these periodic poleward moving PCAs may be triggered by bursts of dayside magnetic reconnection.