Articles | Volume 38, issue 6
https://doi.org/10.5194/angeo-38-1283-2020
https://doi.org/10.5194/angeo-38-1283-2020
Regular paper
 | 
21 Dec 2020
Regular paper |  | 21 Dec 2020

Resolution dependence of magnetosheath waves in global hybrid-Vlasov simulations

Maxime Dubart, Urs Ganse, Adnane Osmane, Andreas Johlander, Markus Battarbee, Maxime Grandin, Yann Pfau-Kempf, Lucile Turc, and Minna Palmroth

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Cited articles

Ahmadi, N., Germaschewski, K., and Raeder, J.: Effects of electron temperature anisotropy on proton mirror instability evolution, J. Geophys. Res.-Space, 121, 5350–5365, https://doi.org/10.1002/2016JA022429, 2016. a, b
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Ala-Lahti, M., Kilpua, E. K. J., Souček, J., Pulkkinen, T. I., and Dimmock, A. P.: Alfvén Ion Cyclotron Waves in Sheath Regions Driven by Interplanetary Coronal Mass Ejections, J. Geophys. Res.-Space, 124, 3893–3909, https://doi.org/10.1029/2019JA026579, 2019. a
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Anderson, B. J. and Fuselier, S. A.: Magnetic pulsations from 0.1 to 4.0 Hz and associated plasma properties in the Earth's subsolar magnetosheath and plasma depletion layer, J. Geophys. Res.Space, 98, 1461–1479, https://doi.org/10.1029/92JA02197, 1993. a, b
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Short summary
Plasma waves are ubiquitous in the Earth's magnetosphere. They are responsible for many energetic processes happening in Earth's atmosphere, such as auroras. In order to understand these processes, thorough investigations of these waves are needed. We use a state-of-the-art numerical model to do so. Here we investigate the impact of different spatial resolutions in the model on these waves in order to improve in the future the model without wasting computational resources.