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SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColombo.
Orsini, S; Livi, S A; Lichtenegger, H; Barabash, S; Milillo, A; De Angelis, E; Phillips, M; Laky, G; Wieser, M; Olivieri, A; Plainaki, C; Ho, G; Killen, R M; Slavin, J A; Wurz, P; Berthelier, J-J; Dandouras, I; Kallio, E; McKenna-Lawlor, S; Szalai, S; Torkar, K; Vaisberg, O; Allegrini, F; Daglis, I A; Dong, C; Escoubet, C P; Fatemi, S; Fränz, M; Ivanovski, S; Krupp, N; Lammer, H; Leblanc, François; Mangano, V; Mura, A; Nilsson, H; Raines, J M; Rispoli, R; Sarantos, M; Smith, H T; Szego, K; Aronica, A; Camozzi, F; Di Lellis, A M; Fremuth, G; Giner, F; Gurnee, R; Hayes, J; Jeszenszky, H; Tominetti, F; Trantham, B.
Afiliação
  • Orsini S; Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy.
  • Livi SA; Southwest Research Institute, San Antonio, TX USA.
  • Lichtenegger H; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA.
  • Barabash S; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Milillo A; Swedish Institute of Space Physics, Kiruna, Sweden.
  • De Angelis E; Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy.
  • Phillips M; Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy.
  • Laky G; Southwest Research Institute, San Antonio, TX USA.
  • Wieser M; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Olivieri A; Swedish Institute of Space Physics, Kiruna, Sweden.
  • Plainaki C; Italian Space Agency, Roma, Italy.
  • Ho G; Italian Space Agency, Roma, Italy.
  • Killen RM; The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA.
  • Slavin JA; NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA.
  • Wurz P; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA.
  • Berthelier JJ; Physics Institute, University of Bern, Bern, Switzerland.
  • Dandouras I; LATMOS/IPSL, CNRS, Sorbonne Université, Paris, France.
  • Kallio E; Institut de Recherche en Astrophysique et Planétologie, CNRS, CNES, Université de Toulouse, Toulouse, France.
  • McKenna-Lawlor S; School of Electrical Engineering, Department of Electronics and Nanoengineering, Aalto University, Helsinki, Finland.
  • Szalai S; Space Technology Ireland, Ltd., Maynooth, Co. Kildare Ireland.
  • Torkar K; Wigner Research Centre for Physics, Budapest, Hungary.
  • Vaisberg O; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Allegrini F; IKI Space Research Institute, Moscow, Russia.
  • Daglis IA; Southwest Research Institute, San Antonio, TX USA.
  • Dong C; Department of Physics, National and Kapodistrian University of Athens, Athens, Greece.
  • Escoubet CP; Hellenic Space Center, Athens, Greece.
  • Fatemi S; Department of Astrophysical Sciences and Princeton Plasma Physics Laboratory, Princeton University, Princeton, NJ USA.
  • Fränz M; ESA-ESTEC, Noordwijk, The Netherlands.
  • Ivanovski S; Swedish Institute of Space Physics, Kiruna, Sweden.
  • Krupp N; Max-Planck-Institut für Sonnensystemforschung, MPS, 37077 Göttingen, Germany.
  • Lammer H; Astronomical Observatory, INAF, Trieste, Italy.
  • Leblanc F; Max-Planck-Institut für Sonnensystemforschung, MPS, 37077 Göttingen, Germany.
  • Mangano V; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Mura A; LATMOS/IPSL, CNRS, Sorbonne Université, Paris, France.
  • Nilsson H; Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy.
  • Raines JM; Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy.
  • Rispoli R; Swedish Institute of Space Physics, Kiruna, Sweden.
  • Sarantos M; Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI USA.
  • Smith HT; Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy.
  • Szego K; NASA/Goddard Space Flight Center, Greenbelt, MD 20771 USA.
  • Aronica A; The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA.
  • Camozzi F; Wigner Research Centre for Physics, Budapest, Hungary.
  • Di Lellis AM; Institute of Space Astrophysics and Planetology, INAF, via del Fosso del Cavaliere 100, 00133 Rome, Italy.
  • Fremuth G; OHB-Italia SpA, Milano, Italy.
  • Giner F; AMDL srl, Roma, Italy.
  • Gurnee R; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Hayes J; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Jeszenszky H; Laboratory for Atmospheric and Space Physics, Boulder, CO USA.
  • Tominetti F; The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723 USA.
  • Trantham B; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
Space Sci Rev ; 217(1): 11, 2021.
Article em En | MEDLINE | ID: mdl-33487762
ABSTRACT
The ESA-JAXA BepiColombo mission to Mercury will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric particle dynamics at Mercury as well as their interactions with solar wind, solar radiation, and interplanetary dust. The particle instrument suite SERENA (Search for Exospheric Refilling and Emitted Natural Abundances) is flying in space on-board the BepiColombo Mercury Planetary Orbiter (MPO) and is the only instrument for ion and neutral particle detection aboard the MPO. It comprises four independent sensors ELENA for neutral particle flow detection, Strofio for neutral gas detection, PICAM for planetary ions observations, and MIPA, mostly for solar wind ion measurements. SERENA is managed by a System Control Unit located inside the ELENA box. In the present paper the scientific goals of this suite are described, and then the four units are detailed, as well as their major features and calibration results. Finally, the SERENA operational activities are shown during the orbital path around Mercury, with also some reference to the activities planned during the long cruise phase.
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Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Space Sci Rev Ano de publicação: 2021 Tipo de documento: Article País de afiliação: Itália
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Space Sci Rev Ano de publicação: 2021 Tipo de documento: Article País de afiliação: Itália