Europlanet Science Congress 2021
Virtual meeting
13 – 24 September 2021
Europlanet Science Congress 2021
Virtual meeting
13 September – 24 September 2021
EPSC Abstracts
Vol. 15, EPSC2021-344, 2021
https://doi.org/10.5194/epsc2021-344
European Planetary Science Congress 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Solar wind protons in the diamagnetic cavity at comet 67P/Churyumov-Gerasimenko

Charlotte Goetz1, Lucie Scharre2, Cyril Simon-Wedlund3, Hans Nilsson4, Elias Odelstad5, Matthew Taylor1, and Martin Volwerk3
Charlotte Goetz et al.
  • 1ESA, ESTEC, Noordwijk, Netherlands (c.goetz@tu-bs.de)
  • 2University of Edinburgh, Old College, South Bridge, Edinburgh EH8 9YL, United Kingdom
  • 3Institut für Weltraumforschung, ÖAW, Graz, Austria
  • 4Institutet för rymdfysik, Kiruna, Sweden
  • 5Institutet för rymdfysik, Uppsala, Sweden

Against expectations, the Rosetta spacecraft was able to observe protons of solar wind origin in the diamagnetic cavity at comet 67P/Churyumov-Gerasimenko. This study investigates these unexpected observations and gives a working hypothesis on what could be the underlying cause.

The cometary plasma environment of a comet is shaped by two distinct plasma populations: the solar wind, consisting of protons, alpha particles, electrons and a magnetic field, and the cometary plasma, consisting of heavy ions such as water ions or carbon dioxide ions and electrons. 
As the comet follows its orbit through the solar system, the amount of cometary ions that is produced varies significantly. This means that the plasma environment of the comet and the boundaries that form there are also dependent on the comet's heliocentric distance. 

For example, at sufficiently high gas production rates (close to the Sun) the protons from the solar wind are prevented from entering the inner coma entirely. The region where no protons (and other solar wind origin ions) can be detected is referred to as the solar wind ion cavity. 
A second example is the diamagnetic cavity, a region very close to the nucleus of the comet, where the interplanetary magnetic field, which is carried by the solar wind electrons, cannot penetrate the densest part of the cometary plasma. 

The Rosetta mission clearly showed that the solar wind ion cavity is larger than the diamagnetic cavity at a comet such as 67P/Churyumov-Gerasimenko. However, this new study finds that in isolated incidences this order can be reversed and ions of solar wind origin (mostly protons, but also helium) can be detected inside the diamagnetic cavity. We present the observations pertaining to these events and list and discard possible mechanisms that could lead to such a configuration. Only one mechanism cannot be discarded: that of a solar wind configuration where the solar wind velocity is aligned with the magnetic field. We show evidence that fits this hypothesis as well as solar wind models in support. 

How to cite: Goetz, C., Scharre, L., Simon-Wedlund, C., Nilsson, H., Odelstad, E., Taylor, M., and Volwerk, M.: Solar wind protons in the diamagnetic cavity at comet 67P/Churyumov-Gerasimenko, European Planetary Science Congress 2021, online, 13–24 Sep 2021, EPSC2021-344, https://doi.org/10.5194/epsc2021-344, 2021.

Display materials

Display link

Comments on the scientific presentation material

to access the discussion