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オゴハラ カズノリ
OGOHARA Kazunori
小郷原 一智 所属 京都産業大学 理学部 宇宙物理・気象学科 職種 准教授 |
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| 言語種別 | 英語 |
| 発行・発表の年月 | 2021/12 |
| 形態種別 | 研究論文 |
| 査読 | 査読あり |
| 標題 | MIRS: an imaging spectrometer for the MMX mission |
| 執筆形態 | 共著 |
| 掲載誌名 | Earth, Planets and Space |
| 掲載区分 | 国外 |
| 巻・号・頁 | 73(1) |
| 国際共著 | 国際共著 |
| 著者・共著者 | Maria Antonietta Barucci,Jean Michel Reess,Pernelle Bernardi,Alain Doressoundiram,Sonia Fornasier,Michel Le Du,Takahiro Iwata,Hiromu Nakagawa,Tomoki Nakamura,Yves André,Shohei Aoki,Takehiko Arai,Elisa Baldit,Pierre Beck,Jean Tristan Buey,Elisabet Canalias,Matthieu Castelnau,Sebastien Charnoz,Marc Chaussidon,Fréderic Chapron,Valerie Ciarletti,Marco Delbo,Bruno Dubois,Stephane Gauffre,Thomas Gautier,Hidenori Genda,Rafik Hassen-Khodja,Gilles Hervet,Ryuki Hyodo,Christian Imbert,Takeshi Imamura,Laure |
| 概要 | The MMX infrared spectrometer (MIRS) is an imaging spectrometer onboard MMX JAXA mission. MMX (Martian Moon eXploration) is scheduled to be launched in 2024 with sample return to Earth in 2029. MIRS is built at LESIA-Paris Observatory in collaboration with four other French laboratories, collaboration and financial support of CNES and close collaboration with JAXA and MELCO. The instrument is designed to fully accomplish MMX’s scientific and measurement objectives. MIRS will remotely provide near-infrared spectral maps of Phobos and Deimos containing compositional diagnostic spectral features that will be used to analyze the surface composition and to support the sampling site selection. MIRS will also study Mars atmosphere, in particular spatial and temporal changes such as clouds, dust and water vapor. Graphical Abstract: [Figure not available: see fulltext.]. |
| DOI | 10.1186/s40623-021-01423-2 |
| ISSN | 1343-8832/1880-5981 |