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Investigating Mercury’s Environment with the Two-Spacecraft BepiColombo Mission

  • A. Milillo*
  • , M. Fujimoto
  • , G. Murakami
  • , J. Benkhoff
  • , J. Zender
  • , S. Aizawa
  • , M. Dósa
  • , L. Griton
  • , D. Heyner
  • , G. Ho
  • , S. M. Imber
  • , X. Jia
  • , T. Karlsson
  • , R. M. Killen
  • , M. Laurenza
  • , S. T. Lindsay
  • , S. McKenna-Lawlor
  • , A. Mura
  • , J. M. Raines
  • , D. A. Rothery
  • N. André, W. Baumjohann, A. Berezhnoy, P. A. Bourdin, E. J. Bunce, F. Califano, J. Deca, S. de la Fuente, C. Dong, C. Grava, S. Fatemi, P. Henri, S. L. Ivanovski, B. V. Jackson, M. James, E. Kallio, Y. Kasaba, E. Kilpua, M. Kobayashi, B. Langlais, F. Leblanc, C. Lhotka, V. Mangano, A. Martindale, S. Massetti, A. Masters, M. Morooka, Y. Narita, J. S. Oliveira, D. Odstrcil, S. Orsini, M. G. Pelizzo, C. Plainaki, F. Plaschke, F. Sahraoui, K. Seki, J. A. Slavin, R. Vainio, P. Wurz, S. Barabash, C. M. Carr, D. Delcourt, K. H. Glassmeier, M. Grande, M. Hirahara, J. Huovelin, O. Korablev, H. Kojima, H. Lichtenegger, S. Livi, A. Matsuoka, R. Moissl, M. Moncuquet, K. Muinonen, E. Quèmerais, Yoshifumi Saito, S. Yagitani, I. Yoshikawa, J. E. Wahlund
*Tämän työn vastaava kirjoittaja
  • Institute of Space and Astronautical Science
  • ESTEC - European Space Research and Technology Centre
  • IRAP
  • Hungarian Academy of Sciences
  • Technical University of Braunschweig
  • Johns Hopkins Applied Physics Laboratory
  • University of Michigan, Ann Arbor
  • University of Leicester
  • KTH Royal Institute of Technology
  • NASA Goddard Space Flight Center
  • Open University Milton Keynes
  • Austrian Academy of Sciences
  • Lomonosov Moscow State University
  • Kazan Federal University
  • University of Graz
  • University of Pisa
  • University of Colorado Boulder
  • Princeton Plasma Physics Laboratory
  • Uppsala University
  • Université d'Orléans
  • INAF, Osservatorio Astronomico di Trieste
  • UC-San-Diego
  • Tohoku University
  • University of Helsinki
  • Chiba Institute of Technology
  • Université de Nantes
  • Sorbonne Université
  • Imperial College London
  • University of Coimbra
  • National Research Council of Italy
  • Agenzia Spaziale Italiana (ASI) Science Data Center, I-00044 Frascati (Roma), Italy
  • The University of Tokyo
  • University of Turku
  • University of Bern
  • Aberystwyth University/Arts Centre
  • Nagoya University
  • Space Research Institute, Russian Academy of Sciences
  • University of Kyoto
  • Observatoire de Paris
  • Université de Versailles Saint-Quentin-en-Yvelines
  • Kanazawa University
  • National Institute for Astrophysics
  • Space Technology Ireland
  • European Space Astronomy Centre
  • Southwest Research Institute

Tutkimustuotos: LehtiartikkeliReview Articlevertaisarvioitu

112 Sitaatiot (Scopus)
151 Lataukset (Pure)

Abstrakti

The ESA-JAXA BepiColombo mission will provide simultaneous measurements from two spacecraft, offering an unprecedented opportunity to investigate magnetospheric and exospheric dynamics at Mercury as well as their interactions with the solar wind, radiation, and interplanetary dust. Many scientific instruments onboard the two spacecraft will be completely, or partially devoted to study the near-space environment of Mercury as well as the complex processes that govern it. Many issues remain unsolved even after the MESSENGER mission that ended in 2015. The specific orbits of the two spacecraft, MPO and Mio, and the comprehensive scientific payload allow a wider range of scientific questions to be addressed than those that could be achieved by the individual instruments acting alone, or by previous missions. These joint observations are of key importance because many phenomena in Mercury’s environment are highly temporally and spatially variable. Examples of possible coordinated observations are described in this article, analysing the required geometrical conditions, pointing, resolutions and operation timing of different BepiColombo instruments sensors.

AlkuperäiskieliEnglanti
Artikkeli93
Sivumäärä78
JulkaisuSpace Science Reviews
Vuosikerta216
Numero5
DOI - pysyväislinkit
TilaJulkaistu - 1 elok. 2020
OKM-julkaisutyyppiA2 Katsausartikkeli tieteellisessä aikakauslehdessä

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