Abstract
Due to the absence of a global intrinsic magnetic field, Mars presents an induced magnetosphere, which is formed by the interaction between the solar wind and the conductive ionosphere of the planet. In that interaction, plasma boundaries and regions are created. Wave activity is present in the Mars plasma environment, and as consequence of non-linear interaction of those fluctuations, turbulence arises in the plasma. In this work, a review of the intermittent plasma turbulence in the upstream and main regions of the induced magnetosphere of Mars is presented. The influence of solar wind dynamic pressure, Mars seasonal variation and the presence of transients in the solar wind on the turbulence and wave activities at Mars are also reported.
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Acknowledgements
A. M. S. F. would like to thank the Institute of Geosciences and Engineering- UNIFESSPA (project no. 23479.018587/2022-14). E. Echer would like to thank Brazilian agencies for research grants: CNPq (contract no. PQ-301883/2019-0). The work of M. J. A. B. was supported by CNPq agency (contract no. PQ-302330/2015-1, PQ-305692/2018-6) and FAPEG agency (contract no. 2012.1026.7000905). We thank the Brazilian Ministry of Science, Technology and Innovation and the Brazilian Space Agency as well. We would like to thank the editor and reviewers for their insightful comments, which have helped us significantly improving our manuscript.
Funding
Work of EE is funded by CNPq (contract no. PQ-302583/2015-7, PQ-301883/2019-0) and FAPESP (2018/21657-1). Work of MJAB is funded by CNPq (contract no. PQ-302330/2015-1, PQ-305692/2018-6) and FAPEG (contract no. 2012.1026.7000905).
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Franco, A.M.S., Echer, E., Fränz, M. et al. Intermittent plasma turbulence in the Martian plasma environment. Rev. Mod. Plasma Phys. 8, 3 (2024). https://doi.org/10.1007/s41614-023-00141-4
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DOI: https://doi.org/10.1007/s41614-023-00141-4