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Solar Orbiter's first Venus flyby MAG observations of structures and waves associated with the induced Venusian magnetosphere

Volwerk, M. (författare)
Austrian Acad Sci, Space Res Inst, Graz, Austria.
Horbury, T. S. (författare)
Imperial Coll London, Dept Phys, Blackett Lab, London, England.
Woodham, L. D. (författare)
Imperial Coll London, Dept Phys, Blackett Lab, London, England.
visa fler...
Bale, S. D. (författare)
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.
Wedlund, C. Simon (författare)
Austrian Acad Sci, Space Res Inst, Graz, Austria.
Schmid, D. (författare)
Austrian Acad Sci, Space Res Inst, Graz, Austria.
Allen, R. C. (författare)
Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA.
Angelini, V (författare)
Imperial Coll London, Dept Phys, Blackett Lab, London, England.
Baumjohann, W. (författare)
Austrian Acad Sci, Space Res Inst, Graz, Austria.
Berger, L. (författare)
Christian Albrechts Univ Kiel, Inst Experimentelle & Angew Phys, Kiel, Germany.
Edberg, Niklas J. T. (författare)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Evans, V (författare)
Imperial Coll London, Dept Phys, Blackett Lab, London, England.
Hadid, L. Z. (författare)
Sorbonne Univ, Univ Paris Saclay, PSL Res Univ, Observ Paris,LPP,CNRS,Ecole Polytech, Paris, France.
Ho, G. C. (författare)
Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA.
Khotyaintsev, Yuri V. (författare)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Magnes, W. (författare)
Austrian Acad Sci, Space Res Inst, Graz, Austria.
Maksimovic, M. (författare)
Sorbonne Univ, Univ Paris Saclay, PSL Res Univ, Observ Paris,LPP,CNRS,Ecole Polytech, Paris, France.
O'Brien, H. (författare)
Imperial Coll London, Dept Phys, Blackett Lab, London, England.
Steller, M. B. (författare)
Austrian Acad Sci, Space Res Inst, Graz, Austria.
Rodriguez-Pacheco, J. (författare)
Univ Alcala De Henares, Space Res Grp, Alcala De Henares, Spain.
Wimmer-Scheingruber, R. F. (författare)
Christian Albrechts Univ Kiel, Inst Experimentelle & Angew Phys, Kiel, Germany.
visa färre...
Austrian Acad Sci, Space Res Inst, Graz, Austria Imperial Coll London, Dept Phys, Blackett Lab, London, England. (creator_code:org_t)
2021-12-14
2021
Engelska.
Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 656
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Context. The induced magnetosphere of Venus is caused by the interaction of the solar wind and embedded interplanetary magnetic field with the exosphere and ionosphere of Venus. Solar Orbiter entered Venus's magnetotail far downstream, > 70 Venus radii, of the planet and exited the magnetosphere over the north pole. This offered a unique view of the system over distances that had only been flown through before by three other missions, Mariner 10, Galileo, and BepiColombo.Aims. In this study, we study the large-scale structure and activity of the induced magnetosphere as well as the high-frequency plasma waves both in the magnetosphere and in a limited region upstream of the planet where interaction with Venus's exosphere is expected.Methods. The large-scale structure of the magnetosphere was studied with low-pass filtered data and identified events are investigated with a minimum variance analysis as well as combined with plasma data. The high-frequency plasma waves were studied with spectral analysis.Results. We find that Venus's magnetotail is very active during the Solar Orbiter flyby. Structures such as flux ropes and reconnection sites were encountered, in addition to a strong overdraping of the magnetic field downstream of the bow shock and planet. High-frequency plasma waves (up to six times the local proton cyclotron frequency) are observed in the magnetotail, which are identified as Doppler-shifted proton cyclotron waves, whereas in the upstream solar wind, these waves appear just below the proton cyclotron frequency (as expected) but are very patchy. The bow shock is quasi-perpendicular, however, expected mirror mode activity is not found directly behind it; instead, there is strong cyclotron wave power. This is most likely caused by the relatively low plasma-beta behind the bow shock. Much further downstream, magnetic hole or mirror mode structures are identified in the magnetosheath.

Ämnesord

NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Nyckelord

planets and satellites
magnetic fields
plasmas

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