日本地球惑星科学連合2019年大会

講演情報

[E] ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS07] アストロバイオロジー

2019年5月30日(木) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:薮田 ひかる(広島大学大学院理学研究科地球惑星システム学専攻)、杉田 精司(東京大学大学院理学系研究科地球惑星科学専攻)、深川 美里(国立天文台)、藤島 皓介(東京工業大学地球生命研究所)

[MIS07-P07] たんぽぽ計画での初期分析のための、機械学習の適用とソフトウエア開発

*奥平 恭子1戸田 悠斗1園家 俊1矢口 勇一1吉田 将司1今仁 順也2佐々木 聰3矢野 創4出村 裕英1田端 誠5山岸 明彦6 (1.会津大学、2.由紀精密、3.東京工科大学、4.宇宙航空研究開発機構、5.千葉大学、6.東京薬科大学)

キーワード:たんぽぽ計画、アストロバイオロジー、初期分析、機械学習、ソフトウエア開発

One of the goals of the TANPOPO mission is collecting cosmic dust and space debris on the International Space Station [1]. Ultra-low density material “silica aerogel” panels are used as capture media [2]. These panels retrieved from the space are sent to the laboratory and initial analysis has been conducted by a system called “CLOXS”.

CLOXS efficiently covers the processes (1) Automatic imaging the entire panel, 2) Search for penetration track candidates, 3) Mapping of track candidates, 4) Shape data acquisition of tracks, and 5) Automatic sample cutting) up to sample allocation to researchers. However, to reduce researchers’ time and effort, improvement of the software and automation of some processes are required.

In this study, application of machine learning in discrimination of objects in aerogel images taken by CLOXS is mainly reported. The research goal is to classify objects in the images into tracks and dirt using machine learning.

There are morphological varieties in the objects. As for both tracks and dirt, they are classified into 4 types respectively in this study.

Since the contrast of the images are low, the first step of our approach is preprocessing of the images. We compared the results of Contrast Stretching and CLAHE (Contrast Limited Adaptive Histogram Equalization).

Learning data and test data are prepared respectively, to compare the case that the images are categorized into 4 types and the case that the images of all types are dealt altogether.

Convolutional Neural Network (CNN) is used as a method of machine learning. Python is used as programing Language.

In conclusion, as for image processing, CLAHE showed higher accuracy when tracks were judged to be tracks, and Contrast Stretching was found to yield a better result for dirt. It is probably because, in Contrast Stretching, CNN was not sufficiently highlighted to capture features, and CLAHE was able to improve the contrast sufficiently.

Regarding separating the types of tracks and dirt, the accuracy rate was higher when tracks were categorized into different types and learned.

Although further evaluation and improvements might be needed, our accuracy rates meet the mission requirements, that is, the percentage of identifying track as track should be more than 95 %, while the percentage of identifying dirt as dirt should be more than 70 % (that of NOT identifying true track as dirt should be less than 30 %).



[1] A. Yamagishi et al., “Tanpopo: Astrobiology exposure and micrometeoroid capture experiments - proposed experiments at the exposure facility of ISS-JEM”, Trans. JSASS. Aerospace Tech. Jpn. vol. 12, No. ists29, p. Tk_49-Tk_55, 2014.

[2] M. Tabata, et al. “Ultralow-density double-layer silica aerogel fabrication for the intact capture of cosmic dust in low-Earth orbits” J. Sol-Gel Sci. Technol. 77(2), 325-334, 2016.