日本地球惑星科学連合2023年大会

講演情報

[E] オンラインポスター発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS03] 太陽系小天体:太陽系の形成と進化における最新成果と今後の展望

2023年5月25日(木) 13:45 〜 15:15 オンラインポスターZoom会場 (1) (オンラインポスター)

コンビーナ:岡田 達明(宇宙航空研究開発機構宇宙科学研究所)、吉田 二美(産業医科大学)、荒川 創太(海洋研究開発機構)、深井 稜汰(宇宙航空研究開発機構)


現地ポスター発表開催日時 (2023/5/24 17:15-18:45)

13:45 〜 15:15

[PPS03-P11] 現在のHEATの開発状況

*金野 龍史1齋藤 啓仁1ラモン ヴィラルデル1荒井 武彦2出村 裕英1 (1.公立大学法人会津大学、2.前橋工科大学)

キーワード:Hera、TIRI、小惑星

HEAT (Hayabusa2/Hera Exploration Assistant for TIR/TIRI) is a calibration tool for thermal imagers; TIR on Hayabusa2 and TIRI on Hera. These imagers observe thermal infrared radiation from small bodies. The primary goal of TIRI/TIRI is to know the origin and evolutional history of asteroids based on thermo-physical properties. We have developed HEAT through the missions of Hayabusa2 and Hera. HEAT has four functions, Calibration, DB, Visualization, and Conversion. The developing HEAT calibrates 1024 * 768 (~ 800,000) pixels of TIRI images one by one. It requires about 100 times the performance of the previous HEAT. The current HEAT has been published on the web page: https://github.com/HEAT-Develop/HEAT. Saito, Master thesis of the University of Aizu (2023), has refactored and updated HEAT to apply another mission by managing metadata with preference files in XML format. Here we will report the new HEAT with ground tests of TIRI based on high-performance computing. We have changed the outputs of the calibration function from a set of coefficients pixel by pixel to a united FITS file. We have updated the interface of the conversion function and applied high-performance computing in a calibration process.

We have changed outputs of calibration function from a set of coefficients pixel by pixel to a united FITS file. We have updated interface of the conversion function, which follows input of FITS file format. We have also applied high performance computing in calibration process.