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

<p>In this work, we investigate magnetic field fluctuations in three coronal mass ejection (CME)-driven sheath regions at 1&thinsp;AU, with their speeds ranging from slow to fast. The data set we use consists primarily of high-resolution (0.092&thinsp;s) magnetic field measurements fro...

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Bibliographic Details
Main Authors: E. K. J. Kilpua, D. Fontaine, S. W. Good, M. Ala-Lahti, A. Osmane, E. Palmerio, E. Yordanova, C. Moissard, L. Z. Hadid, M. Janvier
Format: Article
Language:English
Published: Copernicus Publications 2020-09-01
Series:Annales Geophysicae
Online Access:https://angeo.copernicus.org/articles/38/999/2020/angeo-38-999-2020.pdf