Hybrid modeling of cometary plasma environments. II: Remote-sensing of a cometary bow shock

Research output: Contribution to journalArticleScientificpeer-review


Research units

  • University of Michigan, Ann Arbor
  • University of Oslo
  • Swedish Institute of Space Physics
  • Luleå University of Technology
  • Finnish Meteorological Institute


Context. The ESA Rosetta probe has not seen direct evidence of a fully formed bow shock at comet 67P/Churyumov–Gerasimenko (67P). Ion spectrometer measurements of cometary pickup ions measured in the vicinity of the nucleus of 67P are available and may contain signatures of the large-scale plasma environment.
Aims. The aim is to investigate the possibility of using pickup ion signatures to infer the existence or nonexistence of a bow shock-like structure and possibly other large-scale plasma environment features.
Methods. A numerical plasma model in the hybrid plasma description was used to model the plasma environment of a comet. Simulated pickup ion spectra were generated for different interplanetary magnetic field conditions. The results were interpreted through test particle tracing in the hybrid simulation solutions.
Results. Features of the observed pickup ion energy spectrum were reproduced, and the model was used to interpret the observation to be consistent with a shock-like structure. We identify 1) a spectral break related to the bow shock, 2) a mechanism for generating the spectral break, and 3) a dependency of the e
energy of the spectral break on the interplanetary magnetic field magnitude and bow shock standoff distance.


Original languageEnglish
Number of pages16
JournalAstronomy & Astrophysics
Early online date27 Feb 2019
Publication statusPublished - Oct 2019
MoE publication typeA1 Journal article-refereed

    Research areas

  • Comets: General, comets: individual: 67P, Methods: numerical, Plasmas, shock waves, Techniques: miscellaneous

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