日本地球惑星科学連合2014年大会

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セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS23_2AM2] 月の科学と探査

2014年5月2日(金) 11:00 〜 12:45 413 (4F)

コンビーナ:*諸田 智克(名古屋大学大学院環境学研究科)、本田 親寿(会津大学)、西野 真木(名古屋大学太陽地球環境研究所)、長岡 央(早稲田大学先進理工学部)、座長:長岡 央(早稲田大学先進理工学部)、上本 季更(東京大学大学院理学系研究科地球惑星科学専攻)

11:00 〜 11:15

[PPS23-08] かぐやスペクトルプロファイラデータを動的に解析するためのウェブアプリケーション開発

杉本 紘平1林 洋平2、*小川 佳子1平田 成1寺薗 淳也1出村 裕英1松永 恒雄3山本 聡3横田 康弘3大竹 真紀子4大嶽 久志4 (1.会津大学、2.産総研、3.国環研、4.宇宙研)

Kaguya is a Japanese lunar orbiter launched on September 14, 2007 and observed the moon for about 2 years. The Spectral Profiler (SP) on board Kaguya was a spectrometer which provided global data set of visible-near infrared continuous reflectance spectra of the Moon. GEKKO is a web-application used to visualize the data observed by SP. GEKKO displays the graph of SP spectra and tables of ancillary data with thumbnail images simultaneously taken by Kaguya imager/camera. The current version of GEKKO is very useful for viewing SP spectra, but does not include analysis functions. The goal of this study is to develop a framework for implementing analysis functions of the SP data. For transferring the data from the client, the original GEKKO connects to the server using MapServer. However, in case of MapServer, the client-researchers can only analyze in a predetermined manner. Therefore, we prepared CGI scripts and incorporated them into GEKKO. By using the new GEKKO system, the clients-researchers will be able to dynamically analyze the SP data. The clients can select, coordinate and add the functions according to their objectives. We prepared the basic functions commonly used for the spectral analysis, such as running average, normalization and also similarity measurement.