日本地球惑星科学連合2021年大会

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[J] ポスター発表

セッション記号 M (領域外・複数領域) » M-TT 計測技術・研究手法

[M-TT43] インフラサウンド及び関連波動が繋ぐ多圏融合地球物理学の新描像

2021年6月6日(日) 17:15 〜 18:30 Ch.20

コンビーナ:山本 真行(高知工科大学 システム工学群)、乙津 孝之(一般財団法人 日本気象協会)、市原 美恵(東京大学地震研究所)、新井 伸夫(名古屋大学減災連携研究センター)

17:15 〜 18:30

[MTT43-P04] Infrasound and seismic multiple-site observation of shock waves induced by hypersonic reentry of HAYABUSA-2 sample return capsule on Dec. 6, 2020

*山本 真行1、平松 良浩2、阿部 新助3、柿並 義宏4、瀬川 典久5、片尾 浩6、石原 吉明7、川村 太一8、野澤 恵9、古本 宗充10、Bland Phil11、Sansom Eleanor11、Devillepoix Hadrien11、Towner Martin11、井上 祐一郎1、Hamama Islam1、矢澤 正人12、藤田 和央7、吉川 真7 (1.高知工科大学、2.金沢大学、3.日本大学、4.北海道情報大学、5.京都産業大学、6.京都大学、7.宇宙航空研究開発機構、8.パリ地球物理研究所、9.茨城大学、10.東濃地震科学研究所、11.カーティン大学、12.数理設計研究所)

キーワード:インフラサウンド、衝撃波、多地点アレイ観測、大気圏再突入、はやぶさ2

On Dec. 6, 2020, the JAXA HAYABUSA2 spacecraft returned to the Earth and its sample return capsule (SRC) was successfully landed on the desert area of Woomera, South Australia. At the time of hypersonic reentry of SRC in the upper and middle atmosphere, shock waves can be generated from the Mach cone along the shallow angle trajectory of SRC directly injected from the outer space. In 2010, the HAYABUSA SRC also successfully landed on the ground in the same desert area. At that time, we tried to detect the shock waves coming from the Mach cone of SRC, but little bit different condition that the mother spacecraft also reentered because of the lack of its capability to escape from the Earth's gravity due to the partial malfunction, therefore, multiple shock waves were observed at 5 sensors at that time. Over 20 seismometers simultaneously detected N-type signals with an air-to-ground coupling process at that time, as well (e.g. Yamamoto et al., 2011). After the event, we have been developed new infrasound sensors of INF01 and INF04 with data loggers by ourselves collaborating with some manufacturing companies, thus this time, we can deploy 30 sensors in a 100 km scale target area. Besides, 6 low-cost seismometers were also deployed at 4 sites.

For detecting precise trajectory and yield energy from the dataset of over-pressure amplitude at each site, we deployed 30 sensors on ground in the Woomera Prohibited Area (WPA). As for the INF04 sensors, we used 7 sites using 4 sensors per each, getting N-type waveform at every 27 sensors, except for 1 possible malfunctioned sensor. The waveform was almost the same as the HAYABUSA SRC reentry but without any complex features of the followed period just after the N type signal. The air-to-ground coupling process is also roughly investigated in comparison with previous result in 2010. By using these datasets, we will show the prompt report of the whole of the observation about the infrasound and seismic observation for HAYABUSA2 reentry. The possibility of the yield energy estimation and precise trajectory determination will be discussed in this talk.

Reference:
Yamamoto, M.-Y., Ishihara, Y., Hiramatsu, Y., Kitamura, K., Ueda, M., Shiba, Y., Furumoto, M., Fujita, K., Detection of Acoustic/Infrasonic/Seismic Waves Generated by Hypersonic Re-Entry of the HAYABUSA Capsule and Fragmented Parts of the Spacecraft, Publ. Astron. Soc. Japan, 63, 971-978, 2011.