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SERENA: Particle Instrument Suite for Determining the Sun-Mercury Interaction from BepiColomboThe 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.
Document ID
20220004030
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
S. Orsini
(Institute for Space Astrophysics and Planetology Rome, Italy)
S. A. Livi
(Southwest Research Institute Boulder, CO, United States)
H. Lichtenegger
(Austrian Academy of Sciences Vienna, Austria)
S. Barabash
(Swedish Institute of Space Physics Kiruna, Sweden)
A. Milillo
(Institute for Space Astrophysics and Planetology Rome, Italy)
E. De Angelis
(Institute for Space Astrophysics and Planetology Rome, Italy)
M. Phillips
(Southwest Research Institute Boulder, CO, United States)
G. Laky
(Austrian Academy of Sciences Vienna, Austria)
M. Wieser
(Swedish Institute of Space Physics Kiruna, Sweden)
A. Olivieri
(Italian Space Agency)
C. Plainaki
(Italian Space Agency)
G. Ho
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
R. M. Killen
(Goddard Space Flight Center Greenbelt, Maryland, United States)
J. A. Slavin
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
P. Wu r z
(University of Bern Bern, Switzerland)
J. -J. Berthelier
(Sorbonne Paris Cité Paris, France)
I. Dandouras
(University of Toulouse Toulouse, Midi-Pyrénées, France)
E. Kallio
(Southwest Research Institute Boulder, CO, United States)
S. McKenna-Lawlor
(Space Technology Ireland Ltd Maynooth, Co. Kildare, Ireland)
S. Szalai
(MTA Wigner Research Centre for Physics Budapest, Hungary)
K. Torkar
(Austrian Academy of Sciences Vienna, Austria)
O. Vaisberg
(Space Research Institute Moscow, Russia)
F. Allegrini
(Southwest Research Institute Boulder, CO, United States)
I. A. Daglis
(National and Kapodistrian University of Athens Athens, Attiki, Greece)
C. Dong
(Princeton University Princeton, New Jersey, United States)
C. P. Escoubet
(European Space Research and Technology Centre Noordwijk-Binnen, Netherlands)
S. Fatemi
(Swedish Institute of Space Physics Kiruna, Sweden)
M. Fränz
(Max Planck Institute for Solar System Research Göttingen, Germany)
S. Ivanovski
(Brera Astronomical Observatory Milan, Italy)
N. Krupp
(Max Planck Institute for Solar System Research Göttingen, Germany)
H. Lammer
(Austrian Academy of Sciences Vienna, Austria)
François Leblanc
(Sorbonne University Paris, France)
V. Mangano
(Institute for Space Astrophysics and Planetology Rome, Italy)
A. Mura
(Institute for Space Astrophysics and Planetology Rome, Italy)
H. Nilsson
(Swedish Institute of Space Physics Kiruna, Sweden)
J. M. Raines
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
R. Rispoli
(Institute for Space Astrophysics and Planetology Rome, Italy)
M. Sarantos
(Goddard Space Flight Center Greenbelt, Maryland, United States)
H. T. Smith
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
K. Szego
(MTA Wigner Research Centre for Physics Budapest, Hungary)
A. Aronica
(Institute for Space Astrophysics and Planetology Rome, Italy)
F. Camozzi
(OHB Italia Milano MI, Italy)
A. M. Di Lellis
(University of Michigan–Ann Arbor Ann Arbor, Michigan, United States)
G. Fremuth
(Austrian Academy of Sciences Vienna, Austria)
F. Giner
(Austrian Academy of Sciences Vienna, Austria)
R. Gurnee 2
(Austrian Academy of Sciences Vienna, Austria)
J. Hayes
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
H. Jeszenszky
(Austrian Academy of Sciences Vienna, Austria)
F. Tominetti
(OHB Italia Milano MI, Italy)
B. Trantham
(Southwest Research Institute Boulder, CO, United States)
J. Balaz 2
(Swedish Institute of Space Physics Kiruna, Sweden)
W. Baumjohann
(Austrian Academy of Sciences Vienna, Austria)
D. Brienza
(Institute for Space Astrophysics and Planetology Rome, Italy)
U. Bührke
(Max Planck Institute for Solar System Research Göttingen, Germany)
M. D. Bush
(University of Bern Bern, Switzerland)
M. Cantatore
(OHB Italia Milano MI, Italy)
S. Cibella 2
(Italian Space Agency)
L. Colasanti
(Institute for Space Astrophysics and Planetology Rome, Italy)
G. Cremonese
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
L. Cremonesi
(OHB Italia Milano MI, Italy)
M. D’Alessandro
(Italian Space Agency)
D. Delcourt
(Goddard Space Flight Center Greenbelt, Maryland, United States)
M. Delva
(Austrian Academy of Sciences Vienna, Austria)
M. Desai
(Southwest Research Institute Boulder, CO, United States)
M. Fama
(University of Bern Bern, Switzerland)
M. Ferris
(Southwest Research Institute Boulder, CO, United States)
H. Fischer
(Max Planck Institute for Solar System Research Göttingen, Germany)
A. Gaggero 2
(Italian Space Agency)
D. Gamborino
(University of Bern Bern, Switzerland)
P. Garnier
(University of Toulouse Toulouse, Midi-Pyrénées, France)
W. C . Gibson
(Southwest Research Institute Boulder, CO, United States)
R. Goldstein
(Southwest Research Institute Boulder, CO, United States)
Date Acquired
March 7, 2022
Publication Date
January 12, 2021
Publication Information
Publication: Space Science Reviews
Publisher: Springer
Volume: 217
Issue: 11
Issue Publication Date: January 1, 2021
ISSN: 0038-6308
e-ISSN: 1572-9672
Subject Category
Astrophysics
Funding Number(s)
WBS: 444390.04.02.02
CONTRACT_GRANT: NNG10EK25C
CONTRACT_GRANT: NNG10EK25C
CONTRACT_GRANT: J-090007
CONTRACT_GRANT: SPEC5732
CONTRACT_GRANT: 80NM0018D0004P00002
CONTRACT_GRANT: 1531255
CONTRACT_GRANT: J-090007
CONTRACT_GRANT: 1531255
CONTRACT_GRANT: 1531256
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Keywords
Mercury’s environment
Particle instrumentation
BepiColombo space mission
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