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

被引:9
|
作者
Orsini, S. [1 ]
Milillo, A. [1 ]
Lichtenegger, H. [2 ]
Varsani, A. [2 ]
Barabash, S. [3 ]
Livi, S. [4 ,5 ]
De Angelis, E. [1 ]
Alberti, T. [1 ]
Laky, G. [2 ]
Nilsson, H. [3 ]
Phillips, M. [4 ]
Aronica, A. [1 ]
Kallio, E. [6 ]
Wurz, P. [7 ]
Olivieri, A. [8 ]
Plainaki, C. [8 ]
Slavin, J. A. [5 ]
Dandouras, I. [9 ]
Raines, J. M. [5 ]
Benkhoff, J. [10 ]
Zender, J. [10 ]
Berthelier, J. -J. [11 ]
Dosa, M. [12 ]
Ho, G. C. [13 ]
Killen, R. M. [14 ]
McKenna-Lawlor, S. [15 ]
Torkar, K. [2 ]
Vaisberg, O. [16 ]
Allegrini, F. [4 ,17 ]
Daglis, I. A. [18 ,19 ]
Dong, C. [20 ,21 ]
Escoubet, C. P. [10 ]
Fatemi, S. [22 ]
Fraenz, M. [23 ]
Ivanovski, S. [24 ]
Krupp, N. [23 ]
Lammer, H. [2 ]
Leblanc, Francois
Mangano, V. [1 ]
Mura, A. [1 ]
Rispoli, R. [1 ]
Sarantos, M. [14 ]
Smith, H. T. [13 ]
Wieser, M. [3 ]
Camozzi, F. [25 ]
Di Lellis, A. M. [26 ]
Fremuth, G. [2 ]
Giner, F. [2 ]
Gurnee, R. [27 ]
Hayes, J. [13 ]
机构
[1] INAF, Inst Space Astrophys & Planetol, Rome, Italy
[2] Austrian Acad Sci, Space Res Inst, Graz, Austria
[3] Swedish Inst Space Phys, Kiruna, Sweden
[4] Southwest Res Inst, San Antonio, TX USA
[5] Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI USA
[6] Aalto Univ, Sch Elect Engn, Dept Elect & Nanoengn, Helsinki, Finland
[7] Univ Bern, Inst Phys, Bern, Switzerland
[8] ASI, Italian Space Agcy, Rome, Italy
[9] Univ Toulouse, CNRS, Inst Rech Astrophys & Planetol, CNES, Toulouse, France
[10] ESA ESTEC, Noordwijk, Netherlands
[11] Sorbonne Univ, LATMOS IPSL, CNRS, Paris, France
[12] Wigner Res Ctr Phys, Budapest, Hungary
[13] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[14] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[15] Space Technol Ireland Ltd, Maynooth, Kildare, Ireland
[16] IKI Space Res Inst, Moscow, Russia
[17] Univ Texas San Antonio, Dept Phys & Astron, San Antonio, TX USA
[18] Natl & Kapodistrian Univ Athens, Dept Phys, Athens, Greece
[19] Hellen Space Ctr, Athens, Greece
[20] Princeton Univ, Princeton Plasma Phys Lab, Princeton, NJ USA
[21] Princeton Univ, Dept Astrophys Sci, Princeton, NJ USA
[22] Umea Univ, Dept Phys, Umea, Sweden
[23] MPS, Max Planck Inst Sonnensyst Forsch, D-37077 Gottingen, Germany
[24] INAF, Astron Observ, Trieste, Italy
[25] OHB Italia SpA, Milan, Italy
[26] AMDL Srl, Rome, Italy
[27] Lab Atmospher & Space Phys, Boulder, CO USA
[28] Slovak Acad Sci, Inst Expt Phys SAS, Kosice 04001, Slovakia
[29] Univ Orleans, Orleans, France
[30] Aberystwyth Univ, Aberystwyth, Ceredigion, Wales
[31] Univ Arizona, Tucson, AZ USA
[32] FMI, Helsinki, Finland
[33] Univ Charlottesville, Charlottesville, VA 22904 USA
[34] Ecole Polytech, LPP, F-91128 Palaiseau, France
[35] Univ Tokyo, Dept Earth & Planetary Sci, Grad Sch Sci, Tokyo, Japan
关键词
MAGNETIC-FIELD; MESSENGER; PLASMA; MAGNETOPAUSE;
D O I
10.1038/s41467-022-34988-x
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
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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页数:8
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