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Cited article:

MHD simulation of the solar wind flow around the coma of comet Churyumov–Gerasimenko duringRosetta’s flyby

V B Baranov, D B Alexashov and M G Lebedev
Monthly Notices of the Royal Astronomical Society 482 (4) 5642 (2019)
https://doi.org/10.1093/mnras/sty3080

Influence of the magnetic field on the density distribution of solar wind protons and cometary ions in the shock layer ahead of cometary ionospheres

V. B. Baranov and D. B. Alexashov
Astronomy Letters 43 (2) 126 (2017)
https://doi.org/10.1134/S1063773717020013

Dynamical features and spatial structures of the plasma interaction region of 67P/Churyumov–Gerasimenko and the solar wind

C. Koenders, K.-H. Glassmeier, I. Richter, H. Ranocha and U. Motschmann
Planetary and Space Science 105 101 (2015)
https://doi.org/10.1016/j.pss.2014.11.014

Density distribution of solar wind protons and “loaded” ions in the shock layer ahead of a cometary ionosphere

V. B. Baranov and M. G. Lebedev
Astronomy Letters 40 (10) 648 (2014)
https://doi.org/10.1134/S1063773714100016

Stellar winds and planetary bodies simulations: Lunar type interaction in super-Alfvénic and sub-Alfvénic flows

Y. Vernisse, H. Kriegel, S. Wiehle, U. Motschmann and K.-H. Glassmeier
Planetary and Space Science 84 37 (2013)
https://doi.org/10.1016/j.pss.2013.04.004

Kelvin-Helmholtz instabilities at the magnetic cavity boundary of comet 67P/Churyumov-Gerasimenko

M. Rubin, K. C. Hansen, M. R. Combi, et al.
Journal of Geophysical Research: Space Physics 117 (A6) n/a (2012)
https://doi.org/10.1029/2011JA017300