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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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ANGEO | Articles | Volume 38, issue 5
Ann. Geophys., 38, 999–1017, 2020
https://doi.org/10.5194/angeo-38-999-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 38, 999–1017, 2020
https://doi.org/10.5194/angeo-38-999-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Regular paper 16 Sep 2020

Regular paper | 16 Sep 2020

Magnetic field fluctuation properties of coronal mass ejection-driven sheath regions in the near-Earth solar wind

Emilia K. J. Kilpua et al.

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ED: Publish subject to minor revisions (review by editor) (06 Jul 2020) by Anna Milillo
AR by Adnane Osmane on behalf of the Authors (10 Jul 2020)  Author's response    Manuscript
ED: Publish as is (16 Jul 2020) by Anna Milillo
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Short summary
This paper studies magnetic field fluctuations in three turbulent sheath regions ahead of interplanetary coronal mass ejections (ICMEs) in the near-Earth solar wind. Our results show that fluctuation properties vary significantly in different parts of the sheath when compared to solar wind ahead. Turbulence in sheaths resembles that of the slow solar wind in the terrestrial magnetosheath, e.g. regarding compressibility and intermittency, and it often lacks Kolmogorov's spectral indices.
This paper studies magnetic field fluctuations in three turbulent sheath regions ahead of...
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