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

Kilpua, Emilia K. J.; Fontaine, Dominique; Good, Simon W.; Ala-Lahti, Matti; Osmane, Adnane; Palmerio, Erika; Yordanova, Emiliya; Moissard, Clement; Hadid, Lina Z.; Janvier, Miho

doi:https://doi.org/10.5194/angeo-38-999-2020

Articles | Volume 38, issue 5

https://doi.org/10.5194/angeo-38-999-2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

https://doi.org/10.5194/angeo-38-999-2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 38, issue 5

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, Dominique Fontaine, Simon W. Good, Matti Ala-Lahti, Adnane Osmane, Erika Palmerio, Emiliya Yordanova, Clement Moissard, Lina Z. Hadid, and Miho Janvier

Download

Final revised paper (published on 16 Sep 2020)
Supplement to the final revised paper
Preprint (discussion started on 16 Apr 2020)

Interactive discussion

Status: closed

AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment

- Printer-friendly version

- Supplement

RC1: 'Referee comments on `Magnetic field fluctuation properties of coronal mass ejection-driven sheath regions in the near-Earth solar wind' by E. K. J. Kilpua et al.', Anonymous Referee #1, 20 May 2020
- AC1: 'Response to Reviewer 1 comments', Emilia Kilpua, 25 Jun 2020
RC2: 'Review of Kilpua et al manuscript angel-2020-17', Anonymous Referee #2, 12 Jun 2020
- AC2: 'Response to Reviewer 2 comments', Emilia Kilpua, 25 Jun 2020

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision

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

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.