Energetic ions in the Venusian system: Insights from the first Solar Orbiter flyby

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Fältnamn	Indikatorer	Metadata
000		11425naa a2201153 4500
001		oai:DiVA.org:uu-464272
003		SwePub
008		220119s2021 \| \|\|\|\|\|\|\|\|\|\|\|000 \|\|eng\|
009		oai:DiVA.org:kth-307348
024	7	a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-4642722 URI
024	7	a https://doi.org/10.1051/0004-6361/2021408032 DOI
024	7	a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3073482 URI
040		a (SwePub)uud (SwePub)kth
041		a engb eng
042		9 SwePub
072	7	a ref2 swepub-contenttype
072	7	a art2 swepub-publicationtype
100	1	a Allen, R. C.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.,Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.;Max Planck Inst Solar Syst Res, Gottingen, Germany.4 aut
245	1 0	a Energetic ions in the Venusian system :b Insights from the first Solar Orbiter flyby
264		c 2021-12-14
264	1	b EDP Sciences,c 2021
338		a electronic2 rdacarrier
500		a QC 20220121
520		a The Solar Orbiter flyby of Venus on 27 December 2020 allowed for an opportunity to measure the suprathermal to energetic ions in the Venusian system over a large range of radial distances to better understand the acceleration processes within the system and provide a characterization of galactic cosmic rays near the planet. Bursty suprathermal ion enhancements (up to similar to 10 keV) were observed as far as similar to 50R(V) downtail. These enhancements are likely related to a combination of acceleration mechanisms in regions of strong turbulence, current sheet crossings, and boundary layer crossings, with a possible instance of ion heating due to ion cyclotron waves within the Venusian tail. Upstream of the planet, suprathermal ions are observed that might be related to pick-up acceleration of photoionized exospheric populations as far as 5R(V) upstream in the solar wind as has been observed before by missions such as Pioneer Venus Orbiter and Venus Express. Near the closest approach of Solar Orbiter, the Galactic cosmic ray (GCR) count rate was observed to decrease by approximately 5 percent, which is consistent with the amount of sky obscured by the planet, suggesting a negligible abundance of GCR albedo particles at over 2 R-V. Along with modulation of the GCR population very close to Venus, the Solar Orbiter observations show that the Venusian system, even far from the planet, can be an effective accelerator of ions up to similar to 30 keV. This paper is part of a series of the first papers from the Solar Orbiter Venus flyby.
650	7	a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650	7	a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650	7	a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe
650	7	a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng
653		a acceleration of particles
653		a planets and satellites
653		a terrestrial planets
653		a planet-star interactions
653		a planetary systems
653		a turbulence
653		a waves
700	1	a Cernuda, Iu Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Dimmock, Andrew P.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Tech Univ Dresden, Dresden, Germany.4 aut0 (Swepub:uu)anddi496
700	1	a Berger, L.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.4 aut
700	1	a Xu, Z. G.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.4 aut
700	1	a von Forstner, J. L. Freiherru Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.4 aut
700	1	a Rodriguez-Pacheco, J.u Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Wimmer-Schweingruber, R. F.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.4 aut
700	1	a Ho, G. C.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700	1	a Mason, G. M.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.,Univ Paris Diderot, Observ Paris, Sorbonne Univ, CNRS,LESIA,Univ PSL, Sorbonne Paris Cite,5 Pl Jules Janssen, F-92195 Meudon, France.4 aut
700	1	a Stergiopoulou, Katerinau Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)katst110
700	1	a Khotyaintsev, Yuri V.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)ykh28990
700	1	a Horbury, T.u Imperial Coll, London, England.4 aut
700	1	a Maksimovic, M.u Univ Paris Diderot, Observ Paris, Sorbonne Univ, CNRS,LESIA,Univ PSL, Sorbonne Paris Cite,5 Pl Jules Janssen, F-92195 Meudon, France.,Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.;Max Planck Inst Solar Syst Res, Gottingen, Germany.,Austrian Acad Sci, Space Res Inst, Graz, Austria.,Univ Alcala De Henares, Space Res Grp, Madrid, Spain.,CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.;Univ Orleans, Orleans, France.4 aut
700	1	a Hadid, L. Z.u Univ Paris Saclay, Observ Paris, Sorbonne Univ, Ecole Polytech,CNRS,LPP, Paris, France.4 aut
700	1	a Volwerk, M.u Austrian Acad Sci, Space Res Inst, Graz, Austria.4 aut
700	1	a Dimmock, Andrew P.u Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)anddi496
700	1	a Sorriso-Valvo, Lucau Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,CNR ISTP Ist Sci & Tecnol Plasmi, Via Amendola 122-D, I-70126 Bari, Italy.4 aut0 (Swepub:uu)lucso160
700	1	a Stergiopoulou, Katerinau Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen4 aut0 (Swepub:uu)katst110
700	1	a Andrews, G. B.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700	1	a Angelini, Vu Imperial Coll, London, England.,Univ Paris Diderot, Observ Paris, Sorbonne Univ, CNRS,LESIA,Univ PSL, Sorbonne Paris Cite,5 Pl Jules Janssen, F-92195 Meudon, France.;Radboud Univ Nijmegen, Res Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.4 aut
700	1	a Bale, S. D.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Univ Calif Berkeley, Phys Dept, Berkeley, CA 94720 USA.,Czech Acad Sci, Astron Inst, Prague, Czech Republic.4 aut
700	1	a Boden, S.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.;DSI Datensicherheit GmbH, Rodendamm 34, D-28816 Stuhr, Germany.4 aut
700	1	a Boettcher, S. , I4 aut
700	1	a Chust, T.u Univ Paris Saclay, Observ Paris, Sorbonne Univ, Ecole Polytech,CNRS,LPP, Paris, France.,Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.4 aut
700	1	a Eldrum, S.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.,Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700	1	a Espada, P. P.u Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Lara, F. Espinosau Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Evans, Vu Imperial Coll, London, England.4 aut
700	1	a Gomez-Herrero, R.u Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Hayes, J. R.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700	1	a Hellin, A. M.u Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Kollhoff, A.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.4 aut
700	1	a Krasnoselskikh, Vu CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.4 aut
700	1	a Kretzschmar, M.u CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.;Univ Orleans, Orleans, France.4 aut
700	1	a Kuehl, P.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.4 aut
700	1	a Kulkarni, S. R.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.;Deutsch Elektronen Synchrotron DESY, Platanenallee 6, D-15738 Zeuthen, Germany.4 aut
700	1	a Lees, W. J.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700	1	a Lorfevre, E.u CNES, Toulouse, France.4 aut
700	1	a Martin, C.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.;German Aerosp Ctr, Dept Extrasolar Planets & Atmospheres, Berlin, Germany.4 aut
700	1	a O'Brien, H.u Imperial Coll, London, England.4 aut
700	1	a Plettemeier, D.u Tech Univ Dresden, Dresden, Germany.4 aut
700	1	a Polo, O. R.u Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Prieto, M.u Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Ravanbakhsh, A.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.;Max Planck Inst Solar Syst Res, Gottingen, Germany.4 aut
700	1	a Sanchez-Prieto, S.u Univ Alcala De Henares, Space Res Grp, Madrid, Spain.4 aut
700	1	a Schlemm, C. E.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700	1	a Seifert, H.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.4 aut
700	1	a Soucek, J.u Czech Acad Sci, Inst Atmospher Phys, Prague, Czech Republic.4 aut
700	1	a Steller, M.u Austrian Acad Sci, Space Res Inst, Graz, Austria.4 aut
700	1	a Stverak, S.u Czech Acad Sci, Astron Inst, Prague, Czech Republic.4 aut
700	1	a Terasa, J. C.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.4 aut
700	1	a Travnicek, P.u Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Czech Acad Sci, Astron Inst, Prague, Czech Republic.4 aut
700	1	a Tyagi, K.u Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.;Univ Colorado, LASP, Boulder, CO 80309 USA.4 aut
700	1	a Vaivads, Andrisu KTH,Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Royal Inst Technol, Sch Elect Engn & Comp Sci, Dept Space & Plasma Phys, Stockholm, Sweden.,Rymd- och plasmafysik,Swedish Inst Space Phys IRF, Uppsala, Sweden4 aut0 (Swepub:kth)u167dmzs
700	1	a Vecchio, A.u Univ Paris Diderot, Observ Paris, Sorbonne Univ, CNRS,LESIA,Univ PSL, Sorbonne Paris Cite,5 Pl Jules Janssen, F-92195 Meudon, France.;Radboud Univ Nijmegen, Res Inst Math Astrophys & Particle Phys, Nijmegen, Netherlands.4 aut
700	1	a Yedla, M.u Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.;Max Planck Inst Solar Syst Res, Gottingen, Germany.4 aut
710	2	a Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA.b Christian Albrechts Univ Kiel, Inst Expt & Angewande Phys, D-24118 Kiel, Germany.;Max Planck Inst Solar Syst Res, Gottingen, Germany.4 org
773	0	t Astronomy and Astrophysicsd : EDP Sciencesg 656q 656x 0004-6361x 1432-0746
856	4	u https://doi.org/10.1051/0004-6361/202140803y Fulltext
856	4	u https://uu.diva-portal.org/smash/get/diva2:1630049/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print
856	4	u https://www.aanda.org/articles/aa/pdf/forth/aa40803-21.pdf
856	4 8	u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-464272
856	4 8	u https://doi.org/10.1051/0004-6361/202140803
856	4 8	u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-307348

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Av författaren/redakt...: Allen, R. C.; Cernuda, I; Dimmock, Andrew ...; Berger, L.; Xu, Z. G.; von Forstner, J. ...; visa fler...; Rodriguez-Pachec ...; Wimmer-Schweingr ...; Ho, G. C.; Mason, G. M.; Stergiopoulou, K ...; Khotyaintsev, Yu ...; Horbury, T.; Maksimovic, M.; Hadid, L. Z.; Volwerk, M.; Sorriso-Valvo, L ...; Andrews, G. B.; Angelini, V; Bale, S. D.; Boden, S.; Boettcher, S. , ...; Chust, T.; Eldrum, S.; Espada, P. P.; Lara, F. Espinos ...; Evans, V; Gomez-Herrero, R ...; Hayes, J. R.; Hellin, A. M.; Kollhoff, A.; Krasnoselskikh, ...; Kretzschmar, M.; Kuehl, P.; Kulkarni, S. R.; Lees, W. J.; Lorfevre, E.; Martin, C.; O'Brien, H.; Plettemeier, D.; Polo, O. R.; Prieto, M.; Ravanbakhsh, A.; Sanchez-Prieto, ...; Schlemm, C. E.; Seifert, H.; Soucek, J.; Steller, M.; Stverak, S.; Terasa, J. C.; Travnicek, P.; Tyagi, K.; Vaivads, Andris; Vecchio, A.; Yedla, M.; visa färre...

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