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Inner southern magnetosphere observation of Mercury via SERENA ion sensors in BepiColombo mission.
Orsini, S; Milillo, A; Lichtenegger, H; Varsani, A; Barabash, S; Livi, S; De Angelis, E; Alberti, T; Laky, G; Nilsson, H; Phillips, M; Aronica, A; Kallio, E; Wurz, P; Olivieri, A; Plainaki, C; Slavin, J A; Dandouras, I; Raines, J M; Benkhoff, J; Zender, J; Berthelier, J-J; Dosa, M; Ho, G C; Killen, R M; McKenna-Lawlor, S; Torkar, K; Vaisberg, O; Allegrini, F; Daglis, I A; Dong, C; Escoubet, C P; Fatemi, S; Fränz, M; Ivanovski, S; Krupp, N; Lammer, H; Leblanc, François; Mangano, V; Mura, A; Rispoli, R; Sarantos, M; Smith, H T; Wieser, M; Camozzi, F; Di Lellis, A M; Fremuth, G; Giner, F; Gurnee, R; Hayes, J.
Afiliação
  • Orsini S; Institute of Space Astrophysics and Planetology, INAF, Roma, Italy. stefano.orsini@inaf.it.
  • Milillo A; Institute of Space Astrophysics and Planetology, INAF, Roma, Italy.
  • Lichtenegger H; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Varsani A; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Barabash S; Swedish Institute of Space Physics, Kiruna, Sweden.
  • Livi S; Southwest Research Institute, San Antonio, TX, USA.
  • De Angelis E; University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, USA.
  • Alberti T; Institute of Space Astrophysics and Planetology, INAF, Roma, Italy.
  • Laky G; Institute of Space Astrophysics and Planetology, INAF, Roma, Italy.
  • Nilsson H; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Phillips M; Swedish Institute of Space Physics, Kiruna, Sweden.
  • Aronica A; Southwest Research Institute, San Antonio, TX, USA.
  • Kallio E; Institute of Space Astrophysics and Planetology, INAF, Roma, Italy.
  • Wurz P; Aalto University, Department of Electronics and Nanoengineering, School of Electrical Engineering, Helsinki, Finland.
  • Olivieri A; University of Bern, Institute of Physics, Bern, Switzerland.
  • Plainaki C; Italian Space Agency, ASI, Roma, Italy.
  • Slavin JA; Italian Space Agency, ASI, Roma, Italy.
  • Dandouras I; University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, USA.
  • Raines JM; Institut de Recherche en Astrophysique et Planétologie, CNRS, CNES, Université de Toulouse, Toulouse, France.
  • Benkhoff J; University of Michigan, Department of Climate and Space Sciences and Engineering, Ann Arbor, MI, USA.
  • Zender J; ESA-ESTEC, Noordwijk, The Netherlands.
  • Berthelier JJ; ESA-ESTEC, Noordwijk, The Netherlands.
  • Dosa M; LATMOS/IPSL, CNRS, Sorbonne Université, Paris, France.
  • Ho GC; Wigner Research Centre for Physics, Budapest, Hungary.
  • Killen RM; The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, 20723, USA.
  • McKenna-Lawlor S; NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, USA.
  • Torkar K; Space Technology Ireland, Ltd., Maynooth, Co., Kildare, Ireland.
  • Vaisberg O; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Allegrini F; IKI Space Research Institute, Moscow, Russia.
  • Daglis IA; Southwest Research Institute, San Antonio, TX, USA.
  • Dong C; University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, TX, USA.
  • Escoubet CP; National and Kapodistrian University of Athens, Department of Physics, Athens, Greece.
  • Fatemi S; Hellenic Space Center, Athens, Greece.
  • Fränz M; Princeton Plasma Physics Laboratory and Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA.
  • Ivanovski S; ESA-ESTEC, Noordwijk, The Netherlands.
  • Krupp N; Department of Physics, Umeå University, Umeå, Sweden.
  • Lammer H; Max-Planck-Institut für Sonnensystemforschung, MPS, 37077, Göttingen, Germany.
  • Leblanc F; Astronomincal Observatory, INAF, Trieste, Italy.
  • Mangano V; Max-Planck-Institut für Sonnensystemforschung, MPS, 37077, Göttingen, Germany.
  • Mura A; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
  • Rispoli R; LATMOS/IPSL, CNRS, Sorbonne Université, Paris, France.
  • Sarantos M; Institute of Space Astrophysics and Planetology, INAF, Roma, Italy.
  • Smith HT; Institute of Space Astrophysics and Planetology, INAF, Roma, Italy.
  • Wieser M; Institute of Space Astrophysics and Planetology, INAF, Roma, Italy.
  • Camozzi F; NASA/Goddard Space Flight Center, Greenbelt, MD, 20771, USA.
  • Di Lellis AM; The Johns Hopkins University Applied Physics Laboratory, Laurel, MD, 20723, USA.
  • Fremuth G; Swedish Institute of Space Physics, Kiruna, Sweden.
  • Giner F; OHB-Italia SpA, Milano, Italy.
  • Gurnee R; AMDL srl, Roma, Italy.
  • Hayes J; Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
Nat Commun ; 13(1): 7390, 2022 Nov 30.
Article em En | MEDLINE | ID: mdl-36450728
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.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Nat Commun Assunto da revista: BIOLOGIA / CIENCIA Ano de publicação: 2022 Tipo de documento: Article País de afiliação: Itália

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Nat Commun Assunto da revista: BIOLOGIA / CIENCIA Ano de publicação: 2022 Tipo de documento: Article País de afiliação: Itália