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Sökning: WFRF:(Nilsson Anders G.) > (2020-2024) > The plasma environm...

  • Goetz, CharlotteESTEC, European Space Agency, Keplerlaan 1, AZ Noordwijk, Netherlands; Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle-upon-Tyne, United Kingdom,European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.;Northumbria Univ, Dept Math Phys & Elect Engn, Newcastle Upon Tyne, Tyne & Wear, England. (författare)

The plasma environment of comet 67P/Churyumov-Gerasimenko

  • Artikel/kapitelEngelska2022

Förlag, utgivningsår, omfång ...

  • 2022-11-10
  • Springer,2022
  • electronicrdacarrier

Nummerbeteckningar

  • LIBRIS-ID:oai:DiVA.org:umu-201212
  • https://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-201212URI
  • https://doi.org/10.1007/s11214-022-00931-1DOI
  • https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-489334URI

Kompletterande språkuppgifter

  • Språk:engelska
  • Sammanfattning på:engelska

Ingår i deldatabas

Klassifikation

  • Ämneskategori:ref swepub-contenttype
  • Ämneskategori:for swepub-publicationtype

Anmärkningar

  • Work at Umeå University was supported by the Swedish National Space Agency, grant 108/18.
  • The environment of a comet is a fascinating and unique laboratory to study plasma processes and the formation of structures such as shocks and discontinuities from electron scales to ion scales and above. The European Space Agency's Rosetta mission collected data for more than two years, from the rendezvous with comet 67P/Churyumov-Gerasimenko in August 2014 until the final touch-down of the spacecraft end of September 2016. This escort phase spanned a large arc of the comet's orbit around the Sun, including its perihelion and corresponding to heliocentric distances between 3.8 AU and 1.24 AU. The length of the active mission together with this span in heliocentric and cometocentric distances make the Rosetta data set unique and much richer than sets obtained with previous cometary probes. Here, we review the results from the Rosetta mission that pertain to the plasma environment. We detail all known sources and losses of the plasma and typical processes within it. The findings from in-situ plasma measurements are complemented by remote observations of emissions from the plasma. Overviews of the methods and instruments used in the study are given as well as a short review of the Rosetta mission. The long duration of the Rosetta mission provides the opportunity to better understand how the importance of these processes changes depending on parameters like the outgassing rate and the solar wind conditions. We discuss how the shape and existence of large scale structures depend on these parameters and how the plasma within different regions of the plasma environment can be characterised. We end with a non-exhaustive list of still open questions, as well as suggestions on how to answer them in the future.

Ämnesord och genrebeteckningar

Biuppslag (personer, institutioner, konferenser, titlar ...)

  • Behar, EtienneSwedish Institute of Space Physics, Box 812, Kiruna, Sweden; Lagrange, OCA, UCA, CNRS, Nice, France,Swedish Inst Space Phys, Box 812, S-98128 Kiruna, Sweden.;CNRS, UCA, OCA, Lagrange, Nice, France. (författare)
  • Beth, ArnaudUmeå universitet,Institutionen för fysik,Umeå Univ, Dept Phys, S-90187 Umeå, Sweden.(Swepub:umu)arbb0009 (författare)
  • Bodewits, DennisPhysics Department, Leach Science Center, Auburn University, AL, Auburn, United States,Auburn Univ, Leach Sci Ctr, Phys Dept, Auburn, AL 36832 USA. (författare)
  • Bromley, StevePhysics Department, Leach Science Center, Auburn University, AL, Auburn, United States,Auburn Univ, Leach Sci Ctr, Phys Dept, Auburn, AL 36832 USA. (författare)
  • Burch, JimSouthwest Research Institute, P.O. Drawer 28510, TX, San Antonio, United States,Southwest Res Inst, PO Drawer 28510, San Antonio, TX 78228 USA. (författare)
  • Deca, JanLaboratory for Atmospheric and Space Physics, University of Colorado Boulder, 3665 Discovery Drive, CO, Boulder, United States,Univ Colorado, Lab Atmospher & Space Phys, 3665 Discovery Dr, Boulder, CO 80303 USA. (författare)
  • Divin, AndreyEarth Physics Department, St. Petersburg State University, Ulianovskaya, 1, St Petersburg, Russian Federation,St Petersburg State Univ, Earth Phys Dept, Ulianovskaya 1, St Petersburg 198504, Russia. (författare)
  • Eriksson, Anders I.Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen(Swepub:uu)andeerik (författare)
  • Feldman, Paul D.Department of Physics and Astronomy, Johns Hopkins University, MD, Baltimore, United States,Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA. (författare)
  • Galand, MarinaDepartment of Physics, Imperial College London, Prince Consort Road, London, United Kingdom,Imperial Coll London, Dept Phys, Prince Consort Rd, London SW7 2AZ, England. (författare)
  • Gunell, HerbertUmeå universitet,Institutionen för fysik,Umeå Univ, Dept Phys, S-90187 Umeå, Sweden.(Swepub:umu)hegu0051 (författare)
  • Henri, PierreCNRS, UCA, OCA, Lagrange, Nice, France.;CNRS, LPC2E, Orleans, France. (författare)
  • Heritier, KevinDepartment of Physics, Imperial College London, Prince Consort Road, London, United Kingdom,Imperial Coll London, Dept Phys, Prince Consort Rd, London SW7 2AZ, England. (författare)
  • Jones, Geraint H.UCL Mullard Space Science Laboratory, Holmbury St. Mary, Dorking, United Kingdom; The Centre for Planetary Sciences at UCL/Birkbeck, Gower Street, London, United Kingdom,UCL Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England.;UCL Birkbeck, Ctr Planetary Sci, Gower St, London WC1E 6BT, England. (författare)
  • Mandt, Kathleen E.Johns Hopkins Applied Physics Laboratory, MD, Laurel, United States,Johns Hopkins Appl Phys Lab, Laurel, MD 20728 USA. (författare)
  • Nilsson, HansSwedish Institute of Space Physics, Box 812, Kiruna, Sweden,Swedish Inst Space Phys, Box 812, S-98128 Kiruna, Sweden. (författare)
  • Noonan, John W.Lunar and Planetary Laboratory, University of Arizona, AZ, Tucson, United States,Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85719 USA. (författare)
  • Odelstad, EliasUppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen(Swepub:uu)eliod143 (författare)
  • Parker, Joel W.Southwest Research Institute, CO, Boulder, United States,Southwest Res Inst, Boulder, CO 80302 USA. (författare)
  • Rubin, MartinPhysikalisches Institut, University of Bern, Sidlerstrasse 5, Bern, Switzerland,Univ Bern, Phys Inst, Sidlerstr 5, CH-3012 Bern, Switzerland. (författare)
  • Simon Wedlund, CyrilSpace Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, Graz, Austria,Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria. (författare)
  • Stephenson, PeterDepartment of Physics, Imperial College London, Prince Consort Road, London, United Kingdom,Imperial Coll London, Dept Phys, Prince Consort Rd, London SW7 2AZ, England. (författare)
  • Taylor, Matthew G. G. T.European Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands. (författare)
  • Vigren, ErikUppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen(Swepub:uu)erivi300 (författare)
  • Vines, Sarah K.Johns Hopkins Applied Physics Laboratory, MD, Laurel, United States,Johns Hopkins Appl Phys Lab, Laurel, MD 20723 USA. (författare)
  • Volwerk, MartinSpace Research Institute, Austrian Academy of Sciences, Schmiedlstr. 6, Graz, Austria,Austrian Acad Sci, Space Res Inst, Schmiedlstr 6, A-8042 Graz, Austria. (författare)
  • ESTEC, European Space Agency, Keplerlaan 1, AZ Noordwijk, Netherlands; Department of Mathematics, Physics and Electrical Engineering, Northumbria University, Newcastle-upon-Tyne, United KingdomEuropean Space Agcy, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.;Northumbria Univ, Dept Math Phys & Elect Engn, Newcastle Upon Tyne, Tyne & Wear, England. (creator_code:org_t)

Sammanhörande titlar

  • Ingår i:Space Science Reviews: Springer218:80038-63081572-9672

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