NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Advisory – Planned Maintenance: On Monday, July 15 at 9 PM Eastern the STI Compliance and Distribution Services will be performing planned maintenance on the STI Repository (NTRS) for approximately one hour. During this time users will not be able to access the STI Repository (NTRS).

Back to Results
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
20210000927
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
S. Orsini
(National Institute for Astrophysics Rome, Italy)
S.A. Livi
(Southwest Research Institute San Antonio, Texas, United States)
H. Lichtenegger
(Space Research Institute Graz, Austria)
S. Barabash
(Swedish Institute of Space Physics Kiruna, Sweden)
A. Milillo
(National Institute for Astrophysics Rome, Italy)
E. De Angelis
(National Institute for Astrophysics Rome, Italy)
M. Phillips
(Southwest Research Institute San Antonio, Texas, United States)
G. Laky
(Space Research Institute Graz, Austria)
M. Wieser
(Swedish Institute of Space Physics Kiruna, Sweden)
A. Olivieri
(Agenzia Spaziale Italiana Rome, Italy)
C. Plainaki
(Agenzia Spaziale Italiana Rome, Italy)
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. Wurz
(University of Bern Bern, Switzerland)
J.-J. Berthelier
(Institut Pierre-Simon Laplace Paris, France)
I. Dandouras
(Research Institute in Astrophysics and Planetology Toulouse, France)
E. Kallio
(Aalto University Helsinki, Finland)
S. McKenna-Lawlor
(Space Technology Ireland, Ltd.)
S. Szalai
(MTA Wigner Research Centre for Physics Budapest, Hungary)
K. Torkar
(Space Research Institute Graz, Austria)
O. Vaisberg
(Space Research Institute Moscow, Russia)
F. Allegrini
(Southwest Research Institute San Antonio, Texas, 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
(Trieste Astronomical Observatory Trieste, Italy)
N. Krupp
(Max Planck Institute for Solar System Research Göttingen, Germany)
H. Lammer
(Space Research Institute Graz, Austria)
François Leblanc
(Institut Pierre-Simon Laplace Paris, France)
V. Mangano
(National Institute for Astrophysics Rome, Italy)
A. Mura
(National Institute for Astrophysics 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
(National Institute for Astrophysics 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
(National Institute for Astrophysics Rome, Italy)
F. Camozzi
(OHB (Italy) Milan, Italy)
A.M. Di Lellis
(AMDL Srl)
G. Fremuth
(Space Research Institute Graz, Austria)
F. Giner
(Space Research Institute Graz, Austria)
R. Gurnee
(Laboratory for Atmospheric and Space Physics Boulder, Colorado, United States)
J. Hayes
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
H. Jeszenszky
(Space Research Institute Graz, Austria)
F. Tominetti
(OHB (Italy) Milan, Italy)
B. Trantham
(Southwest Research Institute San Antonio, Texas, United States)
J. Balaz
(Slovak Academy of Sciences Bratislava, Slovakia)
W. Baumjohann
(Space Research Institute Graz, Austria)
D. Brienza
(National Institute for Astrophysics Rome, Italy)
U. Bührke
(Max Planck Institute for Solar System Research Göttingen, Germany)
M.D. Bush
(University of Bern Bern, Switzerland)
M. Cantatore
(OHB (Italy) Milan, Italy)
S. Cibella
(Institute of Structure of Matter Rome, Italy)
L. Colasanti
(National Institute for Astrophysics Rome, Italy)
G. Cremonese
(National Institute for Astrophysics Rome, Italy)
L. Cremonesi
(OHB (Italy) Milan, Italy)
M. D’Alessandro
(Institute of Structure of Matter Rome, Italy)
D. Delcourt
(University of Orléans Orléans, France)
M. Delva
(Space Research Institute Graz, Austria)
M. Desai
(Southwest Research Institute San Antonio, Texas, United States)
M. Fama
(Comisión Nacional de Energía Atómica Buenos Aires, Argentina)
M. Ferris
(Southwest Research Institute San Antonio, Texas, United States)
H. Fischer
(Max Planck Institute for Solar System Research Göttingen, Germany)
A. Gaggero
(Institute of Structure of Matter Rome, Italy)
D. Gamborino
(University of Bern Bern, Switzerland)
P. Garnier
(Research Institute in Astrophysics and Planetology Toulouse, France)
W.C. Gibson
(Southwest Research Institute San Antonio, Texas, United States)
R. Goldstein
(Southwest Research Institute San Antonio, Texas, United States)
M. Grande
(Aberystwyth University Aberystwyth, United Kingdom)
V. Grishin
(Space Research Institute Moscow, Russia)
D. Haggerty
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
M. Holmström
(Swedish Institute of Space Physics Kiruna, Sweden)
I. Horvath
(MTA Wigner Research Centre for Physics Budapest, Hungary)
K.-C. Hsieh
(University of Arizona Tucson, Arizona, United States)
A. Jacques
(Goddard Space Flight Center Greenbelt, Maryland, United States)
R.E. Johnson
(University of Virginia Charlottesville, Virginia, United States)
A. Kazakov
(National Institute for Astrophysics Rome, Italy)
K. Kecskemety
(MTA Wigner Research Centre for Physics Budapest, Hungary)
H. Krüger
(Max Planck Institute for Solar System Research Göttingen, Germany)
C. Kürbisch
(Space Research Institute Graz, Austria)
F. Lazzarotto
(National Institute for Astrophysics Rome, Italy)
Frederic Leblanc
(École Polytechnique Palaiseau, France)
M. Leichtfried
(Space Research Institute Graz, Austria)
R. Leoni
(PRISMA Srl)
A. Loose
(Max Planck Institute for Solar System Research Göttingen, Germany)
D. Maschietti
(Istituto di Fotonica e Nanotecnologie Milan, Italy)
S. Massetti
(National Institute for Astrophysics Rome, Italy)
F. Mattioli
(PRISMA Srl)
G. Miller
(Southwest Research Institute San Antonio, Texas, United States)
D. Moissenko
(Space Research Institute Moscow, Russia)
A. Morbidini
(National Institute for Astrophysics Rome, Italy)
R. Noschese
(National Institute for Astrophysics Rome, Italy)
F. Nuccilli
(National Institute for Astrophysics Rome, Italy)
C. Nunez
(Southwest Research Institute San Antonio, Texas, United States)
N. Paschalidis
(Goddard Space Flight Center Greenbelt, Maryland, United States)
S. Persyn
(Southwest Research Institute San Antonio, Texas, United States)
D. Piazza
(University of Bern Bern, Switzerland)
M. Oja
(Swedish Institute of Space Physics Kiruna, Sweden)
J. Ryno
(Finnish Meteorological Institute Helsinki, Finland)
W. Schmidt
(Finnish Meteorological Institute Helsinki, Finland)
J.A. Scheer
(Tofwerk (Switzerland) Thun, Switzerland)
A. Shestakov
(Space Research Institute Moscow, Russia)
S. Shuvalov
(Space Research Institute Moscow, Russia)
K. Seki
(University of Tokyo Tokyo, Japan)
S. Selci
(Institute of Structure of Matter Rome, Italy)
K. Smith
(Southwest Research Institute San Antonio, Texas, United States)
R. Sordini
(National Institute for Astrophysics Rome, Italy)
J. Svensson
(European Incoherent Scatter Scientific Association Kiruna, Sweden)
L. Szalai
(MTA Wigner Research Centre for Physics Budapest, Hungary)
D. Toublanc
(Research Institute in Astrophysics and Planetology Toulouse, France)
C. Urdiales
(Southwest Research Institute San Antonio, Texas, United States)
A. Varsani
(Space Research Institute Graz, Austria)
N. Vertolli
(National Institute for Astrophysics Rome, Italy)
R. Wallner
(Space Research Institute Graz, Austria)
P. Wahlstroem
(University of Bern Bern, Switzerland)
P. Wilson
(Southwest Research Institute San Antonio, Texas, United States)
S. Zampieri
(National Institute for Astrophysics Rome, Italy)
Date Acquired
January 27, 2021
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
Space Sciences (General)
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
No Preview Available