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Sökning: id:"swepub:oai:DiVA.org:kth-307357" > First-year ion-acou...

First-year ion-acoustic wave observations in the solar wind by the RPW/TDS instrument on board Solar Orbiter

Pisa, D. (författare)
Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic.
Santolik, O. (författare)
Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic.
Hanzelka, M. (författare)
Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic.;Charles Univ Prague, Fac Math & Phys, V Holesovickach 2, Prague 18000 8, Czech Republic.
visa fler...
Nicolaou, G. (författare)
Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic.;Charles Univ Prague, Fac Math & Phys, V Holesovickach 2, Prague 18000 8, Czech Republic.,Southwest Res Inst, San Antonio, TX 78238 USA.;Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England.
Maksimovic, M. (författare)
Southwest Res Inst, San Antonio, TX 78238 USA.;Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England.,Sorbonne Univ, Univ Paris Diderot, Sorbonne Paris Cite, LESIA,Observ Paris,Univ PSL,CNRS, 5 Pl Jules Janssen, F-92195 Meudon, France.,CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.;Univ Orleans, Orleans, France.,Austrian Acad Sci, Space Res Inst, Graz, Austria.
Bale, S. D. (författare)
Sorbonne Univ, Univ Paris Diderot, Sorbonne Paris Cite, LESIA,Observ Paris,Univ PSL,CNRS, 5 Pl Jules Janssen, F-92195 Meudon, France.,Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Univ Calif Berkeley, Phys Dept, Berkeley, CA 94720 USA.,Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic.;Czech Acad Sci, Astron Inst, Prague, Czech Republic.
Chust, T. (författare)
Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA.;Univ Calif Berkeley, Phys Dept, Berkeley, CA 94720 USA.,Univ Paris Saclay, Observ Paris, Sorbonne Univ, Ecole Polytech,LPP,CNRS, Paris, France.
Khotyaintsev, Yuri V. (författare)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Krasnoselskikh, V (författare)
Swedish Inst Space Phys IRF, Uppsala, Sweden.,CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.
Kretzschmar, M. (författare)
CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.
Lorfevre, E. (författare)
CNRS, LPC2E, 3A Ave Rech Sci, Orleans, France.;Univ Orleans, Orleans, France.,CNES, 18 Ave Edouard Belin, F-31400 Toulouse, France.
Plettemeier, D. (författare)
CNES, 18 Ave Edouard Belin, F-31400 Toulouse, France.,Tech Univ Dresden, Wurzburger Str 35, D-01187 Dresden, Germany.
Steller, M. (författare)
Tech Univ Dresden, Wurzburger Str 35, D-01187 Dresden, Germany.
Stverak, S. (författare)
Austrian Acad Sci, Space Res Inst, Graz, Austria.
Travnicek, P. (författare)
Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic.;Czech Acad Sci, Astron Inst, Prague, Czech Republic.,Space Sciences Laboratory, University of California, Berkeley, CA, USA ;Czech Acad Sci, Astron Inst, Prague, Czech Republic.
Vaivads, Andris (författare)
Uppsala universitet,KTH,Rymd- och plasmafysik,Swedish Inst Space Phys IRF, Uppsala, Sweden,Institutet för rymdfysik, Uppsalaavdelningen,Royal Inst Technol, Sch Elect Engn & Comp Sci, Dept Space & Plasma Phys, Stockholm, Sweden.
Vecchio, A. (författare)
Sorbonne Univ, Univ Paris Diderot, Sorbonne Paris Cite, LESIA,Observ Paris,Univ PSL,CNRS, 5 Pl Jules Janssen, F-92195 Meudon, France.;Radboud Univ Nijmegen, Dept Astrophys, Radboud Radio Lab, Nijmegen, Netherlands.,Imperial Coll, Dept Phys, London SW7 2AZ, England.
Horbury, T. (författare)
Imperial Coll, Dept Phys, London SW7 2AZ, England.
O'Brien, H. (författare)
Imperial Coll, Dept Phys, London SW7 2AZ, England.
Evans, V (författare)
Imperial Coll, Dept Phys, London SW7 2AZ, England.
Angelini, V (författare)
Imperial Coll, Dept Phys, London SW7 2AZ, England.
Owen, C. J. (författare)
Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England.
Louarn, P. (författare)
Inst Rech Astrophys & Planetol, 9 Ave Colonel Roche,BP 4346, F-31028 Toulouse 4, France.
Souček, J. (författare)
Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic.;Charles Univ Prague, Fac Math & Phys, V Holesovickach 2, Prague 18000 8, Czech Republic.
visa färre...
Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic Czech Acad Sci, Inst Atmospher Phys, Bocni 2 1401, Prague 14100, Czech Republic.;Charles Univ Prague, Fac Math & Phys, V Holesovickach 2, Prague 18000 8, Czech Republic. (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. Electric field measurements of the Time Domain Sampler (TDS) receiver, part of the Radio and Plasma Waves (RPW) instrument on board Solar Orbiter, often exhibit very intense broadband wave emissions at frequencies below 20 kHz in the spacecraft frame. During the first year of the mission, the RPW/TDS instrument was operating from the first perihelion in mid-June 2020 and through the first flyby of Venus in late December 2020. Aims. In this paper, we present a year-long study of electrostatic fluctuations observed in the solar wind at an interval of heliocentric distances from 0.5 to 1 AU. The RPW/TDS observations provide a nearly continuous data set for a statistical study of intense waves below the local plasma frequency. Methods. The on-board and continuously collected and processed properties of waveform snapshots allow for the mapping plasma waves at frequencies between 200 Hz and 20 kHz. We used the triggered waveform snapshots and a Doppler-shifted solution of the dispersion relation for wave mode identification in order to carry out a detailed spectral and polarization analysis. Results. Electrostatic ion-acoustic waves are the most common wave emissions observed between the local electron and proton plasma frequency by the TDS receiver during the first year of the mission. The occurrence rate of ion-acoustic waves peaks around perihelion at distances of 0.5 AU and decreases with increasing distances, with only a few waves detected per day at 0.9 AU. Waves are more likely to be observed when the local proton moments and magnetic field are highly variable. A more detailed analysis of more than 10 000 triggered waveform snapshots shows the mean wave frequency at about 3 kHz and wave amplitude about 2.5 mV m(-1). The wave amplitude varies as R-1.38 with the heliocentric distance. The relative phase distribution between two components of the E-field projected in the Y - Z Spacecraft Reference Frame (SRF) plane shows a mostly linear wave polarization. Electric field fluctuations are closely aligned with the directions of the ambient field lines. Only a small number (3%) of ion-acoustic waves are observed at larger magnetic discontinuities.

Ämnesord

NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Nyckelord

waves
solar wind
plasmas
instabilities

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ref (ämneskategori)
art (ämneskategori)

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