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.Menura: a code for simulating the interaction between a turbulent solar wind and solar system bodies
Related authors
Related subject area
Subject: Magnetosphere & space plasma physics | Keywords: Planetary magnetospheres
Ionospheric density depletions around crustal fields at Mars and their connection to ion frictional heating
Reconstruction of Mercury's internal magnetic field beyond the octupole
Ann. Geophys., 42, 69–78,
2024Ann. Geophys., 40, 91–105,
2022Cited 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