JpGU-AGU Joint Meeting 2017

講演情報

[EE] 口頭発表

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-EM11] [EE] Mesosphere-Thermosphere-Ionosphere Coupling in the Earth's Atmosphere

2017年5月24日(水) 13:45 〜 15:15 A01 (東京ベイ幕張ホール)

コンビーナ:Chang Loren(Institute of Space Science, National Central University)、Liu Huixin(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)、齊藤 昭則(京都大学大学院理学研究科地球物理学教室)、Tzu-Wei Fang、座長:齊藤 昭則(Kyoto University, Japan)

13:45 〜 14:05

[PEM11-16] Energetic particle impact on the Na layer

★招待講演

*津田 卓雄1高橋 透2野澤 悟徳3川原 琢也4川端 哲也3斎藤 徳人5和田 智之5Hall Chris6小川 泰信2細川 敬祐1中村 卓司2江尻 省2西山 尚典2阿保 真7津野 克彦5Gumbel Jörg8Hedin Jonas8 (1.電気通信大学、2.国立極地研究所、3.名古屋大学、4.信州大学、5.理化学研究所、6.ノルウェー北極大学、7.首都大学東京、8.ストックホルム大学)

キーワード:Na layer, energetic particle precipitation, auroral activity

The metallic atom and ion layers, its source is considered as ablation of meteoroids coming into the atmosphere, are generally distributed mainly height range of 80-110 km or higher in the upper atmosphere. An importance of the metallic ions, such as Na+ and Fe+, is their longer chemical lifetimes, i.e. slower recombination rates, compared with major ions, such as NO+ and O2+. This can contribute to maintain dens electron concentration, which can influence radio propagation in the upper atmosphere, e.g., satellite communication between the ground and space. The metallic atoms, such as Na and Fe, are also important as a reservoir of the metallic ions through their chemical processes. Thus, it is socially important to investigate the metallic atom and ion layers for understanding or prediction of the radio propagation environment in the upper atmosphere.

In this presentation, we will introduce our recent investigation, which focuses on energetic particle impact on the Na layer. There are several previous studies on this issue. Of interest is that the previous studies reported conflicting results and/or suggestions in the response of Na density to auroral activity. In some cases the Na density increased, and in others it decreased. Thus, the Na density response to auroral activity is still unclear. We have been working on this issue using ground-based observations, such as Na resonance scattering lidar and European incoherent scatter (EISCAT) radar, as well as Na dayglow measurements from space, such as Optical Spectrograph and InfraRed Imager System (OSIRIS) onboard the Odin satellite. As the results of our investigation, we conclude that the basic auroral effect to the Na density is a decrease not an increase and the decrease is probably induced through Na ion chemistry triggered by ionization due to energetic particle precipitation related with the auroral activity.