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Ion acoustic waves near a comet nucleus : Rosetta observations at comet 67P/Churyumov-Gerasimenko

Gunell, Herbert (author)
Umeå universitet,Institutionen för fysik,Umeå Univ, Dept Phys, S-90187 Umeå, Sweden.
Goetz, Charlotte (author)
European Space Agcy, Space Res & Technol Ctr, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands.,Space Research and Technology Centre, European Space Agency, Keplerlaan 1, Noordwijk, Netherlands
Odelstad, Elias (author)
KTH,Rymd- och plasmafysik,Department of Space and Plasma Physics, Royal Institute of Technology, Stockholm, Sweden,Royal Inst Technol, Dept Space & Plasma Phys, S-10044 Stockholm, Sweden.
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Beth, Arnaud (author)
Umeå universitet,Institutionen för fysik,Umeå Univ, Dept Phys, S-90187 Umeå, Sweden.
Hamrin, Maria, 1972- (author)
Umeå universitet,Institutionen för fysik,Umeå Univ, Dept Phys, S-90187 Umeå, Sweden.
Henri, Pierre (author)
CNRS, LPC2E, F-45071 Orleans, France.;UCA, CNRS, OCA, Lagrange, Nice, France.
Johansson, Fredrik (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen,Institutionen för fysik och astronomi,Swedish Inst Space Phys, Box 537, S-75121 Uppsala, Sweden.
Nilsson, Hans (author)
Swedish Inst Space Phys, Box 812, S-98128 Kiruna, Sweden.,Swedish Institute of Space Physics, Box 812, Kiruna, Sweden
Wieser, Gabriella Stenberg (author)
Swedish Inst Space Phys, Box 812, S-98128 Kiruna, Sweden.,Swedish Institute of Space Physics, Box 812, Kiruna, Sweden
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 (creator_code:org_t)
2021-01-15
2021
English.
In: Annales Geophysicae. - : Copernicus GmbH. - 0992-7689 .- 1432-0576. ; 39:1, s. 53-68
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Ion acoustic waves were observed between 15 and 30 km from the centre of comet 67P/Churyumov-Gerasimenko by the Rosetta spacecraft during its close flyby on 28 March 2015. There are two electron populations: one cold at k(B)T(e) approximate to 0.2 eV and one warm at k(B)T(e) approximate to 2 eV. The ions are dominated by a cold (a few hundredths of electronvolt) distribution of water group ions with a bulk speed of (3-3.7) km s(-1). A warm k(B)T(e) approximate to 6 eV ion population, which also is present, has no influence on the ion acoustic waves due to its low density of only 0.25 % of the plasma density. Near closest approach the propagation direction was within 50 degrees from the direction of the bulk velocity. The waves, which in the plasma frame appear below the ion plasma frequency f(pi) approximate to 2 kHz, are Doppler-shifted to the spacecraft frame where they cover a frequency range up to approximately 4 kHz. The waves are detected in a region of space where the magnetic field is piled up and draped around the inner part of the ionised coma. Estimates of the current associated with the magnetic field gradient as observed by Rosetta are used as input to calculations of dispersion relations for current-driven ion acoustic waves, using kinetic theory. Agreement between theory and observations is obtained for electron and ion distributions with the properties described above. The wave power decreases over cometocentric distances from 24 to 30 km. The main difference between the plasma at closest approach and in the region where the waves are decaying is the absence of a significant current in the latter. Wave observations and theory combined supplement the particle measurements that are difficult at low energies and complicated by spacecraft charging.

Subject headings

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

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