JpGU-AGU Joint Meeting 2017

講演情報

[JJ] 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-EM22] [JJ] 大気圏・電離圏

2017年5月24日(水) 13:45 〜 15:15 ポスター会場 (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)

[PEM22-P01] Spatial and temporal variations of upper mesospheric winds inferred by using successive images of noctilucent clouds observed in Iceland.

山下 遼馬1、*鈴木 秀彦1 (1.明治大学理工学部物理学科)

キーワード:夜光雲、風速場、中間圏界面、上部中間圏

Injection of momentum through dissipations of gravity waves propagated from lower atmosphere and active productions of minor constituents caused by precipitation of energetic particles are known as dominant sources of disturbances in upper mesosphere. Since some of these disturbances occur locally and intermittently, it is important to know time constant (i.e. diffusivity) against such impulsive fluctuations on momentum and concentration of minor constituents to understand the energy and mass budgets in the upper mesosphere. One of the straight methods to know the amplitude of the eddy diffusion is to measure the spatial distribution of wind field with high temporal resolution. In this study, derivation of spatial and temporal variation of upper mesospheric winds by tracking a motion of noctilucent cloud (NLC) observed by a ground-based color digital camera in Iceland is conducted. The procedure for wind field estimation consists with 3 steps; (1) projects raw images to a geographical map (2) enhances NLC structures by using FFT method (3) determines horizontal velocity vectors by applying template matching method to two sequential images. In this talk, a result of the wind derivation by using successive images of NLC with 3 minutes interval and ~1.5h duration observed on the night of Aug 1st, 2013 will be reported as a case study.