# Plasma waves at comet 67P/Churyumov-Gerasimenko: in the diamagnetic cavity and outside it

Herbert Gunell, Kathrin Altwegg, Gaël Cessateur, Johan de Keyser, Frederik Dhooghe, Anders Eriksson, Andrew Gibbons, Karl-Heinz Glassmeier, Charlotte Goetz, Tomas Karlsson, et al.

► To cite this version:

Herbert Gunell, Kathrin Altwegg, Gaël Cessateur, Johan de Keyser, Frederik Dhooghe, et al. Plasma waves at comet 67P/Churyumov-Gerasimenko: in the diamagnetic cavity and outside it. 19th EGU General Assembly, Apr 2017, Vienne, Austria. pp.7796. insu-03568147

HAL Id: insu-03568147

https://insu.hal.science/insu-03568147

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# Plasma waves at comet 67P/Churyumov-Gerasimenko: in the diamagnetic cavity and outside it

Herbert Gunell (1), Kathrin Altwegg (2), Gaël Cessateur (1), Johan De Keyser (1), Frederik Dhooghe (1), Anders Eriksson (3), Andrew Gibbons (1,10), Karl-Heinz Glassmeier (4), Charlotte Goetz (4), Tomas Karlsson (5), Maria Hamrin (6), Pierre Henri (7), Romain Maggiolo (1), Hans Nilsson (8), Elias Odelstad (3,11), Martin Rubin (2), Cyril Simon Wedlund (9), Gabriella Stenberg Wieser (8), Chia-Yu Tzou (2), and Xavier Vallieres (7)

(1) Royal Belgian Institute for Space Aeronomy, Bruxelles, Belgium (herbert.gunell@physics.org), (2) Physikalisches Institut, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland, (3) Swedish Institute of Space Physics, Ångström Laboratory, Lägerhyddsvägen 1, Uppsala, Sweden, (4) Institut für Geophysik und extraterrestrische Physik, TU Braunschweig, Mendelssohnstr. 3, 38106 Braunschweig, Germany, (5) Space and Plasma Physics, School of Electrical Engineering, KTH Royal Institute of Technology, Stockholm, Sweden, (6) Department of Physics, Umeå University, 901 87 Umeå, Sweden, (7) LPC2E, CNRS, Orléans, France, (8) Swedish Institute of Space Physics, Box 812, 981 28 Kiruna, Sweden, (9) Department of Physics, University of Oslo, Box 1048 Blindern, 0316 Oslo, Norway, (10) Laboratoire de Chimie Quantique et Photophysique, Université Libre de Bruxelles, 50 Avenue F. D. Roosevelt, B-1050 Brussels, Belgium, (11) Department of Physics and Astronomy, Uppsala University, SE-75120 Uppsala, Sweden

We present observations of waves at Comet 67P/Churyumov-Gerasimenko performed on 20 January 2015, when the activity of the comet was low, and in July and August 2015 when the activity had increased and the Rosetta spacecraft passed through the diamagnetic cavity several times.

We use distribution functions obtained by the Ion Composition Analyser of the Rosetta Plasma Consortium (RPC-ICA) and electron temperature estimates from the Langmuir Probes (RPC-LAP) to compute dispersion relations for waves on the ion timescale, and we compare the results to spectra obtained by RPC-LAP.

On 20 January 2015, at low activity, peaks of the wave spectra appeared at frequencies near 500 Hz, and we identify these waves as ion acoustic. We performed cross-calibrations between RPC-ICA, RPC-LAP, and the Mutual Impedance Probe (RPC-MIP) in order to determine the plasma density. Matching the dispersion relations to the wave observations also helps us estimating the density. We explore the relationship between the waves, the ion distribution functions, and the neutral density, which was measured by the ROSINA-COPS instrument. It is found that when the waves are seen, the ion temperature is low (approximately 0.01 eV). At times the ion temperature is higher (approximately 1 eV), approaching the electron temperature, which leads to strong damping of the ion acoustic waves. This happens when the neutral density is high, suggesting that the ions are heated by being accelerated by the solar wind electric field and scattered in collisions with the neutrals.

These results are compared to measurements of wave spectra when Rosetta was inside the diamagnetic cavity in July and August 2015. In the cavity, the plasma is effectively unmagnetised. We identify cavity passages using the magnetometer RPC-MAG. The waves are analysed in the same way as in the earlier measurements outside the cavity, and the two cases are compared.