JpGU-AGU Joint Meeting 2020

講演情報

[E] 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] 大気圏ー電離圏結合

コンビーナ:Huixin Liu(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Yue Deng(University of Texas at Arlington)、Loren Chang(Institute of Space Science, National Central University)

[PEM12-P02] Relationship between Na layer and CNA variations observed over Syowa, Antarctic

*津田 卓雄1戸津 亮1滝沢 響吾1田中 良昌2川原 琢也3江尻 省2西山 尚典2中村 卓司2 (1.電気通信大学、2.国立極地研究所、3.信州大学)

キーワード:Na 層、CNA、ライダー

Metallic layers, such as Na, Fe, Mg, K, and Ca layers, exist in the mesosphere and lower thermosphere, that correspond to the height range of the ionospheric D and E regions. In the polar region, energetic particles precipitating from the magnetosphere can often penetrate into the E region and even into the D region. Therefore, the influence of energetic particles on the metallic layers is of interest regarding changes in atmospheric composition accompanied by auroral activity or geomagnetic activity.

In this study, we have performed a statistical data analysis on Na layer responses to geomagnetic activity using Na density data, together with simultaneous cosmic noise absorption (CNA) data, obtained at Syowa, Antarctic (69.0ºS, 39.6ºE) in 2000-2002. It is found that the Na densities around the topside of Na layers tended to decrease during geomagnetic active days, but in contrast the CNA tended to increase. The amounts of Na density responses, i.e., Na density decrease or Na loss, were increasing with magnetic local time (MLT) from dusk hours to dawn hours, and those of CNA responses, i.e., CNA increase, were also increasing with MLT. Thus, there were clear negative correlations between the Na density and the CNA variations. These results indicate that the the Na loss around the topside of Na layer was induced by the energetic particle precipitation during geomagnetic active days.