日本地球惑星科学連合2019年大会

講演情報

[J] 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-EM16] 大気圏・電離圏

2019年5月29日(水) 10:45 〜 12:15 A03 (東京ベイ幕張ホール)

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)、座長:大塚 雄一江尻 省(国立極地研究所)

11:00 〜 11:15

[PEM16-08] 高分解能Ca+ライダーによって観測されたスポラディックE層の微細構造

*江尻 省1,2中村 卓司1,2津田 卓雄3西山 尚典1,2阿保 真4高橋 透1津野 克彦5川原 琢也6小川 貴代5和田 智之5 (1.国立極地研究所、2.総合研究大学院大学、3.電気通信大学、4.首都大学東京、5.理化学研究所光量子工学研究センター、6.信州大学工学部)

キーワード:共鳴散乱ライダー、カルシウムイオン密度、スポラディックE層、微細構造、中間圏・下部熱圏領域

The vertical fine structures and the time evolution of plasma irregularities in the sporadic E (Es) layer were observed via calcium ion (Ca+) density measurements using a resonance scattering lidar with a high time-height resolution (5 s and 15 m) at Tachikawa (35.7°N, 139.4°E) on December 24, 2014. The observation successfully provided clearer fine structures of plasma irregularities, such as quasi-sinusoidal variation, localized clumps, “cats-eye” structures, and twist structures, in the sporadic Ca+ (Ca+s) layers at around 100 km altitude. These fine structures suggested that the Kelvin-Helmholtz (K-H) instabilities occurred in the neutral atmosphere whose density changed temporarily or spatially. The maximum Ca+ density in the Ca+s layer was two orders of magnitude smaller than the maximum electron density estimated from the critical frequency (foEs) observed by the ionosonde at Kokubunji (35.7°N, 139.5°E) simultaneously. The correlation showed a strong positive correlation with a coefficient of 0.91. These results suggest that Ca+ contributes forming the Es layer as well as major metallic ions Fe+ and Mg+ in the lower thermosphere. Moreover, the formation of a new Ca+s layer at 110 km and the upward motions of the Ca+s layers at 100 km and 110 km were observed just after the sunrise time at the conjugation point and before the local sunrise. Although the presence or absence of a causal relationship with the sunrise time was not clear, a possible explanation for the formation and the upward motions of the Ca+s layers was the occurrence of strong eastward winds at around 100 km, rather than the enhancement of the eastward electric field.