Pre-flight Calibration and Near-Earth Commissioning Results of the Mercury Plasma Particle Experiment (MPPE) Onboard MMO (Mio)
Autor: | Jean-Jacques Berthelier, Henning Fischer, Mathieu Petiot, Kazushi Asamura, Eric Le Comte, Zdenĕk Nĕmec̆ek, Andrei Fedorov, Giuseppe Consolini, Yoichi Kazama, Haruhisa Matsumoto, Yoshizumi Miyoshi, Christian Mazelle, Kanako Seki, Jean Rouzaud, Christophe Verdeil, Dominique Delcourt, Wataru Miyake, Harald Michalik, F. Leblanc, Björn Fiethe, Ulrich Bührke, Roberto Bruno, Peter Wurz, Iannis Dandouras, Alain Barthe, Henry-Claude Séran, Jean-André Sauvaud, Maria Federica Marcucci, Mats Holmström, Stas Barabash, Shoichiro Yokota, H. Andersson, Joachim Woch, Masahiro Hoshino, Iku Shinohara, Philippe Louarn, Benoit Lavraud, Dominique Fontaine, Vincent Génot, Alexandre Cadu, Yuki Harada, Christian Jacquey, Anne-Marie Frezoul, Andrew J. Coates, Bruno Katra, Yoshifumi Futaana, Emmanuel Penou, Stefan Karlsson, Jean-Marie Illiano, Markus Fraenz, Claude Aoustin, Qiugang Zong, Catherine Garat, Qiu-Mei Lee, Wing-Huen Ip, Manabu Shimoyama, Masaki N. Nishino, David Moirin, Norbert Krupp, Nicolas André, Masaki Fujimoto, Mitsuo Oka, Hiroshi Hasegawa, Martin Wieser, Guy Peyre, Jana Safrankova, Jean-Louis Médale, Kunihiro Keika, Jean-Denis Techer, Takeshi Takashima, T. Yanagimachi, Naoki Terada, Takefumi Mitani, Masafumi Hirahara, Yoshifumi Saito |
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Přispěvatelé: | Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency [Sagamihara] (JAXA), Laboratoire de Physique des Plasmas (LPP), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-École polytechnique (X)-Sorbonne Université (SU)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Institute for Space-Earth Environmental Research [Nagoya] (ISEE), Nagoya University, Swedish Institute of Space Physics [Kiruna] (IRF), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Osaka University [Osaka], Space Sciences Laboratory [Berkeley] (SSL), University of California [Berkeley] (UC Berkeley), University of California (UC)-University of California (UC), Kyoto University, AKKA Technologies, Institut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Société MICROTEC, Nexeya Conseil & Formation, COMAT, Faculty of Mathematics and Physics [Charles University of Praha], Charles University [Prague] (CU), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Tokai University, The University of Tokyo (UTokyo), Mullard Space Science Laboratory (MSSL), University College of London [London] (UCL), HELIOS - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), Max-Planck-Gesellschaft, Institute of Computer and Network Engineering [Braunschweig] (IDA), Technische Universität Braunschweig = Technical University of Braunschweig [Braunschweig], Japan Aerospace Exploration Agency [Tsukuba] (JAXA), Rikkyo University [Tokyo], Peking University [Beijing], University of Bern, Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), Academia Sinica, National Central University [Taiwan] (NCU), Tohoku University [Sendai], Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), University of California [Berkeley], University of California-University of California, Kyoto University [Kyoto], Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS), Max-Planck-Institut für Sonnensystemforschung (MPS) |
Jazyk: | angličtina |
Rok vydání: | 2021 |
Předmět: |
Spectrum analyzer
High energy particle 010504 meteorology & atmospheric sciences [PHYS.ASTR.EP]Physics [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP] chemistry.chemical_element 7. Clean energy 01 natural sciences law.invention Orbiter law 0103 physical sciences Calibration Aerospace engineering 010303 astronomy & astrophysics 0105 earth and related environmental sciences [PHYS]Physics [physics] Energetic neutral atom Spacecraft business.industry Astronomy and Astrophysics Mercury (element) Solar wind chemistry 13. Climate action Space and Planetary Science [SDU]Sciences of the Universe [physics] Environmental science business [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
Zdroj: | Space Science Reviews Space Science Reviews, 2021, 217 (5), pp.70. ⟨10.1007/s11214-021-00839-2⟩ Space Science Reviews, Springer Verlag, 2021, 217 (5), pp.70. ⟨10.1007/s11214-021-00839-2⟩ Space Science Reviews, Springer Verlag, 2021, 217 (5), ⟨10.1007/s11214-021-00839-2⟩ |
ISSN: | 0038-6308 1572-9672 |
DOI: | 10.1007/s11214-021-00839-2⟩ |
Popis: | International audience; BepiColombo Mio (previously called MMO: Mercury Magnetospheric Orbiter) was successfully launched by Ariane 5 from Kourou, French Guiana on October 20, 2018. The Mercury Plasma/Particle Experiment (MPPE) is a comprehensive instrument package onboard Mio spacecraft used for plasma, high-energy particle and energetic neutral atom measurements. It consists of seven sensors including two Mercury Electron Analyzers (MEA1 and MEA2), Mercury Ion Analyzer (MIA), Mass Spectrum Analyzer (MSA), High Energy Particle instrument for electron (HEP-ele), High Energy Particle instrument for ion (HEP-ion), and Energetic Neutrals Analyzer (ENA). Significant efforts were made pre-flight to calibrate all of the MPPE sensors at the appropriate facilities on the ground. High voltage commissioning of MPPE analyzers was successfully performed between June and August 2019 and in February 2020 following the completion of the low voltage commissioning in November 2018. Although all of the MPPE analyzers are now ready to begin observation, the full service performance has been delayed until Mio’s arrival at Mercury. Most of the fields of view (FOVs) of the MPPE analyzers are blocked by the thermal shield surrounding the Mio spacecraft during the cruising phase. Together with other instruments on Mio including Magnetic Field Investigation (MGF) and Plasma Wave Investigation (PWI) that measure plasma field parameters, MPPE will contribute to the comprehensive understanding of the plasma environment around Mercury when BepiColombo/Mio begins observation after arriving at the planet Mercury in December 2025. |
Databáze: | OpenAIRE |
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