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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00010822naa a2200949 4500
001oai:DiVA.org:uu-464278
003SwePub
008220117s2021 | |||||||||||000 ||eng|
009oai:DiVA.org:kth-307352
024a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-4642782 URI
024a https://doi.org/10.1051/0004-6361/2021409342 DOI
024a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3073522 URI
040 a (SwePub)uud (SwePub)kth
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Hadid, L. Z.u PSL Res Univ, LPP, CNRS, Observ Paris,Sorbonne Univ,Ecole Polytech,Inst Po, F-91120 Palaiseau, France.4 aut
2451 0a Solar Orbiter's first Venus flyby :b Observations from the Radio and Plasma Wave instrument
264 c 2021-12-14
264 1b EDP Sciences,c 2021
338 a electronic2 rdacarrier
500 a QC 20220124
520 a Context. On December 27, 2020, Solar Orbiter completed its first gravity assist manoeuvre of Venus (VGAM1). While this flyby was performed to provide the spacecraft with sufficient velocity to get closer to the Sun and observe its poles from progressively higher inclinations, the Radio and Plasma Wave (RPW) consortium, along with other operational in situ instruments, had the opportunity to perform high cadence measurements and study the plasma properties in the induced magnetosphere of Venus.Aims. In this paper, we review the main observations of the RPW instrument during VGAM1. They include the identification of a number of magnetospheric plasma wave modes, measurements of the electron number densities computed using the quasi-thermal noise spectroscopy technique and inferred from the probe-to-spacecraft potential, the observation of dust impact signatures, kinetic solitary structures, and localized structures at the bow shock, in addition to the validation of the wave normal analysis on-board from the Low Frequency Receiver.Methods. We used the data products provided by the different subsystems of RPW to study Venus' induced magnetosphere.Results. The results include the observations of various electromagnetic and electrostatic wave modes in the induced magnetosphere of Venus: strong emissions of similar to 100 Hz whistler waves are observed in addition to electrostatic ion acoustic waves, solitary structures and Langmuir waves in the magnetosheath of Venus. Moreover, based on the different levels of the wave amplitudes and the large-scale variations of the electron number densities, we could identify different regions and boundary layers at Venus.Conclusions. The RPW instrument provided unprecedented AC magnetic and electric field measurements in Venus' induced magnetosphere for continuous frequency ranges and with high time resolution. These data allow for the conclusive identification of various plasma waves at higher frequencies than previously observed and a detailed investigation regarding the structure of the induced magnetosphere of Venus. Furthermore, noting that prior studies were mainly focused on the magnetosheath region and could only reach 10-12 Venus radii (R-V) down the tail, the particular orbit geometry of Solar Orbiter's VGAM1, allowed the first investigation of the nature of the plasma waves continuously from the bow shock to the magnetosheath, extending to similar to 70R(V) in the far distant tail region.
650 7a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a plasmas
653 a waves
653 a polarization
700a Edberg, Niklas J. T.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)niked861
700a Chust, T.u PSL Res Univ, LPP, CNRS, Observ Paris,Sorbonne Univ,Ecole Polytech,Inst Po, F-91120 Palaiseau, France.4 aut
700a Dimmock, Andrew P.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Tech Univ Dresden, Warzburger Str 35, D-01187 Dresden, Germany.4 aut0 (Swepub:uu)anddi496
700a Dimmock, Andrew P.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)anddi496
700a Morooka, Michikou Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Univ PSL, Sorbonne Univ, Univ Paris, Observ Paris,LESIA,CNRS, Meudon, France.,Univ Orleans, CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.,Austrian Acad Sci, Space Res Inst, Graz, Austria.,Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.,Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA.,Radboud Univ Nijmegen, Radboud Radio Lab, Dept Astrophys, Nijmegen, Netherlands.,Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA.,CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA.4 aut0 (Swepub:uu)mimor108
700a Maksimovic, M.u Univ PSL, Sorbonne Univ, Univ Paris, Observ Paris,LESIA,CNRS, Meudon, France.4 aut
700a Khotyaintsev, Yuri V.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)ykh28990
700a Soucek, J.u Czech Acad Sci, Dept Space Phys, Inst Atmospher Phys, Prague, Czech Republic.4 aut
700a Kretzschmar, M.u Univ Orleans, CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.4 aut
700a Vecchio, A.u Univ PSL, Sorbonne Univ, Univ Paris, Observ Paris,LESIA,CNRS, Meudon, France.;Radboud Univ Nijmegen, Radboud Radio Lab, Dept Astrophys, Nijmegen, Netherlands.,Imperial Coll, Dept Phys, London SW7 2AZ, England.4 aut
700a Le Contel, O.u PSL Res Univ, LPP, CNRS, Observ Paris,Sorbonne Univ,Ecole Polytech,Inst Po, F-91120 Palaiseau, France.4 aut
700a Retino, A.u PSL Res Univ, LPP, CNRS, Observ Paris,Sorbonne Univ,Ecole Polytech,Inst Po, F-91120 Palaiseau, France.,Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700a Allen, R. C.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700a Volwerk, M.u Austrian Acad Sci, Space Res Inst, Graz, Austria.4 aut
700a Fowler, C. M.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.4 aut
700a Sorriso-Valvo, Lucau Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,CNR, Ist Sci & Tecnol Plasmi ISTP, Via Amendola 122-D, I-70126 Bari, Italy.4 aut0 (Swepub:uu)lucso160
700a Karlsson, Tomas,d 1964-u KTH,Rymd- och plasmafysik,KTH Royal Inst Technol, Space & Plasma Phys, S-10405 Stockholm, Sweden.4 aut0 (Swepub:kth)u154ti5p
700a Santolik, O.u Czech Acad Sci, Dept Space Phys, Inst Atmospher Phys, Prague, Czech Republic.;Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.4 aut
700a Kolmasova, Iu Czech Acad Sci, Dept Space Phys, Inst Atmospher Phys, Prague, Czech Republic.;Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic.,Univ PSL, Sorbonne Univ, Univ Paris, Observ Paris,LESIA,CNRS, Meudon, France.4 aut
700a Sahraoui, F.u PSL Res Univ, LPP, CNRS, Observ Paris,Sorbonne Univ,Ecole Polytech,Inst Po, F-91120 Palaiseau, France.4 aut
700a Stergiopoulou, Katerinau Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)katst110
700a Moussas, X.u Natl & Kapodistrian Univ Athens, Dept Astrophys Astron & Mech, Fac Phys, Sch Sci, Zografos 15783, Greece.4 aut
700a Issautier, K.u Univ PSL, Sorbonne Univ, Univ Paris, Observ Paris,LESIA,CNRS, Meudon, France.4 aut
700a Dewey, R. M.u Univ Michigan, Dept Climate & Space Sci & Engn, Ann Arbor, MI 48109 USA.4 aut
700a Wolt, M. Kleinu Radboud Univ Nijmegen, Radboud Radio Lab, Dept Astrophys, Nijmegen, Netherlands.4 aut
700a Malandraki, O. E.u Natl Observ Athens, IAASARS, Metaxa & Vas Pavlou Str, Athens 15236, Greece.4 aut
700a Kontar, E. P.u Univ Glasgow, Sch Phys & Astron, Glasgow G12 8QQ, Lanark, Scotland.4 aut
700a Howes, G. G.u Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA.4 aut
700a Bale, S. D.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA.,Czech Acad Sci, Astron Inst, Prague, Czech Republic.;Czech Acad Sci, Inst Atmospher Phys, Prague, Czech Republic.4 aut
700a Horbury, T. S.u Imperial Coll, Dept Phys, London SW7 2AZ, England.4 aut
700a Martinovic, M.u Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA.4 aut
700a Vaivads, Andrisu Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Sch Elect Engn & Comp, Dept Space & Plasma Phys, Stockholm, Sweden.4 aut0 (Swepub:uu)anvai517
700a Krasnoselskikh, Vu Univ Orleans, CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.4 aut
700a Lorfevre, E.u CNES, 18 Ave Edouard Belin, F-31400 Toulouse, France.4 aut
700a Plettemeier, D.u Tech Univ Dresden, Warzburger Str 35, D-01187 Dresden, Germany.4 aut
700a Steller, M.u Austrian Acad Sci, Space Res Inst, Graz, Austria.4 aut
700a Stverak, S.u Czech Acad Sci, Astron Inst, Prague, Czech Republic.;Czech Acad Sci, Inst Atmospher Phys, Prague, Czech Republic.4 aut
700a Travnicek, P.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Czech Acad Sci, Inst Atmospher Phys, Prague, Czech Republic.4 aut
700a O'Brien, H.u Imperial Coll, Dept Phys, London SW7 2AZ, England.4 aut
700a Evans, Vu Imperial Coll, Dept Phys, London SW7 2AZ, England.4 aut
700a Angelini, Vu Imperial Coll, Dept Phys, London SW7 2AZ, England.4 aut
700a Velli, M. C.u CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA.4 aut
700a Zouganelis, Iu European Space Agcy ESA, European Space Astron Ctr ESAC, Camino Bajo Castillo S-N, Madrid 28692, Spain.4 aut
710a PSL Res Univ, LPP, CNRS, Observ Paris,Sorbonne Univ,Ecole Polytech,Inst Po, F-91120 Palaiseau, France.b Institutet för rymdfysik, Uppsalaavdelningen4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 656q 656x 0004-6361x 1432-0746
856u https://doi.org/10.1051/0004-6361/202140934y Fulltext
856u https://uu.diva-portal.org/smash/get/diva2:1629152/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print
856u https://www.aanda.org/articles/aa/pdf/forth/aa40934-21.pdf
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-464278
8564 8u https://doi.org/10.1051/0004-6361/202140934
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-307352

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