Inner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission

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作者
S. Orsini
A. Milillo
H. Lichtenegger
A. Varsani
S. Barabash
S. Livi
E. De Angelis
T. Alberti
G. Laky
H. Nilsson
M. Phillips
A. Aronica
E. Kallio
P. Wurz
A. Olivieri
C. Plainaki
J. A. Slavin
I. Dandouras
J. M. Raines
J. Benkhoff
J. Zender
J.-J. Berthelier
M. Dosa
G. C. Ho
R. M. Killen
S. McKenna-Lawlor
K. Torkar
O. Vaisberg
F. Allegrini
I. A. Daglis
C. Dong
C. P. Escoubet
S. Fatemi
M. Fränz
S. Ivanovski
N. Krupp
H. Lammer
François Leblanc
V. Mangano
A. Mura
R. Rispoli
M. Sarantos
H. T. Smith
M. Wieser
F. Camozzi
A. M. Di Lellis
G. Fremuth
F. Giner
R. Gurnee
J. Hayes
机构
[1] INAF,Institute of Space Astrophysics and Planetology
[2] Austrian Academy of Sciences,Space Research Institute
[3] Swedish Institute of Space Physics,Institut de Recherche en Astrophysique et Planétologie, CNRS
[4] Southwest Research Institute,LATMOS/IPSL, CNRS
[5] University of Michigan,Princeton Plasma Physics Laboratory and Department of Astrophysical Sciences
[6] Department of Climate and Space Sciences and Engineering,Department of Physics
[7] Aalto University,Institute of Experimental Physics SAS
[8] Department of Electronics and Nanoengineering,undefined
[9] School of Electrical Engineering,undefined
[10] University of Bern,undefined
[11] Institute of Physics,undefined
[12] Italian Space Agency,undefined
[13] ASI,undefined
[14] CNES,undefined
[15] Université de Toulouse,undefined
[16] ESA-ESTEC,undefined
[17] Sorbonne Université,undefined
[18] Wigner Research Centre for Physics,undefined
[19] The Johns Hopkins University Applied Physics Laboratory,undefined
[20] NASA/Goddard Space Flight Center,undefined
[21] Space Technology Ireland,undefined
[22] Ltd.,undefined
[23] Maynooth,undefined
[24] Co.,undefined
[25] IKI Space Research Institute,undefined
[26] University of Texas at San Antonio,undefined
[27] Department of Physics and Astronomy,undefined
[28] National and Kapodistrian University of Athens,undefined
[29] Department of Physics,undefined
[30] Hellenic Space Center,undefined
[31] Princeton University,undefined
[32] Umeå University,undefined
[33] Max-Planck-Institut für Sonnensystemforschung,undefined
[34] MPS,undefined
[35] Astronomincal Observatory,undefined
[36] INAF,undefined
[37] OHB-Italia SpA,undefined
[38] AMDL srl,undefined
[39] Laboratory for Atmospheric and Space Physics,undefined
[40] Slovak Academy of Sciences,undefined
[41] Universitè d’Orleans,undefined
[42] Aberystwyth University,undefined
[43] University of Arizona,undefined
[44] Finnish Meteorological Institute FMI,undefined
[45] University of Virginia,undefined
[46] LPP,undefined
[47] École polytechnique,undefined
[48] University of Tokyo,undefined
[49] Department of Earth and Planetary Science,undefined
[50] Graduate School of Science,undefined
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摘要
Mercury’s southern inner magnetosphere is an unexplored region as it was not observed by earlier space missions. In October 2021, BepiColombo mission has passed through this region during its first Mercury flyby. Here, we describe the observations of SERENA ion sensors nearby and inside Mercury’s magnetosphere. An intermittent high-energy signal, possibly due to an interplanetary magnetic flux rope, has been observed downstream Mercury, together with low energy solar wind. Low energy ions, possibly due to satellite outgassing, were detected outside the magnetosphere. The dayside magnetopause and bow-shock crossing were much closer to the planet than expected, signature of a highly eroded magnetosphere. Different ion populations have been observed inside the magnetosphere, like low latitude boundary layer at magnetopause inbound and partial ring current at dawn close to the planet. These observations are important for understanding the weak magnetosphere behavior so close to the Sun, revealing details never reached before.
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