日本地球惑星科学連合2018年大会

講演情報

[JJ] 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-EM18] 大気圏・電離圏

2018年5月22日(火) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 7ホール)

コンビーナ:大塚 雄一(名古屋大学宇宙地球環境研究所)、津川 卓也(情報通信研究機構)、川村 誠治(国立研究開発法人 情報通信研究機構)

[PEM18-P04] Study on geomagnetic responses of Na, Mg, and Mg+ layers based on Envisat/SCIAMACHY observations

*津田 卓雄1Burrows John2von Savigny Christian3Langowski Martin3中村 卓司4江尻 省4西山 尚典4 (1.電気通信大学、2.University of Bremen、3.University of Greifswald、4.国立極地研究所)

キーワード:金属原子層、金属イオン層、オーロラ活動、Envisat/SCIAMACHY

Metallic atom layers and metallic ion layers, such as Na, Mg, and Mg+ layers, exist in the mesosphere and lower thermosphere (MLT). The height range in the MLT region corresponds to the ionospheric D and E regions. Further, in the polar regions, the energetic particles precipitating from the magnetosphere can often penetrate into the E region and even into the D region. Consequently, the influence of energetic particles on the metallic layers is of interest regarding changes in the atmospheric composition accompanying auroral activity or geomagnetic activity.

In this study, we investigated the geomagnetic responses in the Na, Mg, and Mg+ layers using the SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY (SCIAMACHY) onboard the Envisat. The results showed a significant decrease in the Na density at heights above 95 km at latitudes above 50ºS during geomagnetically active periods. In contrast, a significant increase in the Mg+ density was found at heights above 105 km at latitudes above 40ºS during geomagnetically active periods. The most probable explanation for the Na and Mg+ responses is the charge-transfer reactions triggered by ionization due to energetic particle precipitation during geomagnetically active periods.