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-P02] 南米パタゴニアにおける近赤外カメラによる大気重力波観測

*鈴木 臣1中村 卓司2江尻 省2津野 克彦3西山 尚典2水野 亮4Salvador Jacobo5,6,7 (1.愛知大学地域政策学部、2.国立極地研究所、3.理化学研究所、4.名古屋大学宇宙地球環境研究所、5.Laser Application Research Center (CEILAP)–UNIDEF (MINDEF-CONICET)、6.Universidad Tecnológica Nacional, Facultad Regional Buenos Aires、7.Universidad Nacional de la Patagonia Austral)

Atmospheric gravity waves significantly contribute to the wind/thermal structures in the mesosphere and lower thermosphere (MLT) through their vertical transport of horizontal momentum. It has been reported that the gravity wave momentum flux preferentially associated with the scale of the waves. Airglow imaging is a useful technique to observe two-dimensional structure of small-scale (<100 km) gravity waves in the MLT region and has been used to investigate global behaviour of the waves. In the Southern hemisphere, however, the observations of the MLT gravity waves are very limited compared to those in the Northern hemisphere.
The ANtarctic Gravity Wave Instrument Network (ANGIWN) project has started in 2011 to understand gravity waves over the Antarctic and the effects on general circulation. It is known that the southern Andes is a hot spot of gravity waves and would also contribute significantly to the dynamics in the upper atmosphere. We installed all-sky camera to monitor the MLT gravity waves in November 2017 at Rio Gallegos station (51.6S, 69.3W), Patagonia, Argentina, as an extension the ANGWIN network. The Patagonia camera has an InGaAs array sensor, which is sensitive to the near-infrared (900-1700 nm), and can image OH Meinel band airglow (height: ~85 km) without interference filter, obtaining an OH airglow image every 5 s with an exposure time of 2 s. The system is similar to the imagers of ANGWIN network at Davis, McMurdo, Halley, Syowa and the south-pole. We expect that the airglow imaging at this site would contribute to reveal the characteristic of gravity waves generated around the hot spot at Andes and Antarctic Peninsula.
In this presentation, we will report the design of the observation system and some initial results.