Articles | Volume 40, issue 3
https://doi.org/10.5194/angeo-40-281-2022
© Author(s) 2022. This work is distributed under the Creative Commons Attribution 4.0 License.
Regular paper
| 
09 May 2022
Regular paper |
| 09 May 2022
| 09 May 2022
Menura: a code for simulating the interaction between a turbulent solar wind and solar system bodies
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Subject: Magnetosphere & space plasma physics | Keywords: Planetary magnetospheres
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Ann. Geophys., 40, 91–105, 2022
Cited articles
Alfven, H. t.: On the theory of comet tails, Tellus, 9, 92–96, 1957. a
Bagdonat, T. and Motschmann, U.: 3D Hybrid Simulation Code Using Curvilinear
Coordinates, J. Comput. Phys., 183, 470–485,
https://doi.org/10.1006/jcph.2002.7203, 2002. a, b
Behar, E.: Menura, Zenodo [code], https://doi.org/10.5281/zenodo.6517018, 2022 (code available at: https://gitlab.com/etienne.behar/menura, last access: 3 May 2022). a
Behar, E., Tabone, B., Saillenfest, M., Henri, P., Deca, J., Lindkvist, J.,
Holmström, M., and Nilsson, H.: Solar wind dynamics around a comet-A 2D
semi-analytical kinetic model, Astron. Astrophys., 620, A35, https://doi.org/10.1051/0004-6361/201832736, 2018. a
Boldyrev, S., Perez, J. C., Borovsky, J. E., and Podesta, J. J.: Spectral
scaling laws in magnetohydrodynamic turbulence simulations and
in the solar wind, Astrophys. J., 741, L19,
https://doi.org/10.1088/2041-8205/741/1/l19, 2011. a
