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Investigating Mercury's Environment with the Two-Spacecraft BepiColombo Mission 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 MES-SENGER 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.
Document ID
20210009784
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
A. Milillo ORCID
(Institute for Space Astrophysics and Planetology Rome, Italy)
M. Fujimoto
(Japan Aerospace Exploration Agency Tokyo, Japan)
G. Murakami
(Japan Aerospace Exploration Agency Tokyo, Japan)
J. Benkhoff
(European Space Agency, ESTEC Noordwijk, Netherlands)
J. Zender
(European Space Agency, ESTEC Noordwijk, Netherlands)
S. Aizawa
(University of Toulouse Toulouse, Midi-Pyrénées, France)
M. Dósa
(MTA Wigner Research Centre for Physics Budapest, Hungary)
L. Griton
(University of Toulouse Toulouse, Midi-Pyrénées, France)
D. Heyner
(Technische Universität Braunschweig Braunschweig, Germany)
G. Ho
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
S. M. Imber
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
X. Jia
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
T. Karlsson
(Royal Institute of Technology Stockholm, Sweden)
R. M. Killen
(Goddard Space Flight Center Greenbelt, Maryland, United States)
M. Laurenza
(Institute for Space Astrophysics and Planetology Rome, Italy)
S. T. Lindsay
(University of Leicester Leicester, United Kingdom)
S. McKenna-Lawlor
(Space Technology Ireland, Ltd.)
A. Mura
(Institute for Space Astrophysics and Planetology Rome, Italy)
J. M. Raines
(ARC-NAS-HECC Ann Arbor, Michigan, United States)
D. A. Rothery
(The Open University)
N. André
(University of Toulouse Toulouse, Midi-Pyrénées, France)
W. Baumjohann
(Space Research Institute Graz, Austria)
A. Berezhnoy
(Moscow State University Moscow, Russia)
P. A. Bourdin
(Space Research Institute Graz, Austria)
E. J. Bunce
(University of Leicester Leicester, United Kingdom)
F. Califano
(University of Pisa Pisa, Toscana, Italy)
J. Deca
(University of Colorado Boulder Boulder, Colorado, United States)
S. de la Fuente
(European Space Astronomy Centre Madrid, Spain)
C. Dong
(Princeton University Princeton, New Jersey, United States)
C. Grava
(Southwest Research Institute San Antonio, Texas, United States)
S. Fatemi
(Swedish Institute of Space Physics Kiruna, Sweden)
P. Henri
(University of Orléans Orléans, France)
S. L. Ivanovski
(INFN Sezione di Trieste Trieste, Italy)
B. V. Jackson
(University of California, San Diego San Diego, California, United States)
M. James
(University of Leicester Leicester, United Kingdom)
E. Kallio
(Aalto University Helsinki, Finland)
Y. Kasaba
(Tohoku University Sendai, Japan)
E. Kilpua
(University of Helsinki Helsinki, Finland)
M. Kobayashi
(Chiba Institute of Technology Narashino, Japan)
B. Langlais
(University of Nantes Nantes, France)
F. Leblanc
(Sorbonne University Paris, France)
C. Lhotka
(Space Research Institute Graz, Austria)
V. Mangano
(Institute for Space Astrophysics and Planetology Rome, Italy)
A. Martindale
(University of Leicester Leicester, United Kingdom)
S. Massetti
(Institute for Space Astrophysics and Planetology Rome, Italy)
A. Masters
(Imperial College London London, Westminster, United Kingdom)
M. Morooka
(Swedish Institute of Space Physics Kiruna, Sweden)
Y. Narita
(University of Graz Graz, Steiermark, Austria)
J. S. Oliveira
(European Space Agency, ESTEC Noordwijk, Netherlands)
D. Odstrcil
(Goddard Space Flight Center Greenbelt, Maryland, United States)
S. Orsini
(Institute for Space Astrophysics and Planetology Rome, Italy)
M. G. Pelizzo
(Institute for Photonics and Nanotechnologies)
C. Plainaki
(Italian Space Agency)
F. Plaschke
(Space Research Institute Graz, Austria)
F. Sahraoui
(Laboratoire de Physique des Plasmas Palaiseau, France)
K. Seki
(University of Tokyo)
J. A. Slavin
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
R. Vainio
(University of Turku Turku, Finland)
P. Wurz
(University of Bern Bern, Switzerland)
S. Barabash
(Swedish Institute of Space Physics Kiruna, Sweden)
C. M. Carr
(Imperial College London London, Westminster, United Kingdom)
D. Delcourt
(University of Orléans Orléans, France)
K.-H. Glassmeier
(Technische Universität Braunschweig Braunschweig, Germany)
M. Grande
(Aberystwyth University Aberystwyth, United Kingdom)
M. Hirahara
(Nagoya University Nagoya, Japan)
J. Huovelin
(University of Helsinki Helsinki, Finland)
O. Korablev
(Space Research Institute Moscow, Russia)
H. Kojima
(Kyoto University Kyoto, Japan)
H. Lichtenegger
(Space Research Institute Graz, Austria)
S. Livi
(Southwest Research Institute San Antonio, Texas, United States)
A. Matsuoka
(Japan Aerospace Exploration Agency Tokyo, Japan)
R. Moissl
(European Space Agency, ESTEC Noordwijk, Netherlands)
M. Moncuquet
(Laboratory of Space Studies and Instrumentation in Astrophysics Meudon, France)
K. Muinonen
(University of Helsinki Helsinki, Finland)
E. Quèmerais
(Versailles Saint-Quentin-en-Yvelines University Versailles, France)
Y. Saito
(Japan Aerospace Exploration Agency Tokyo, Japan)
S. Yagitani
(Kanazawa University Kanazawa, Japan)
I. Yoshikawa
(University of Tokyo)
J.-E. Wahlund
(Swedish Institute of Space Physics Kiruna, Sweden)
Date Acquired
February 4, 2021
Publication Date
July 14, 2020
Publication Information
Publication: Space Science Reviews
Publisher: Springer
Volume: 216
ISSN: 0038-6308
e-ISSN: 1572-9672
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
WBS:  444390.04.02.02
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
External Peer Committee
Keywords
Mercury's environment
Magnetosphere
Exosphere
BepiColombo
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