Articles | Volume 38, issue 2
Regular paper
 | Highlight paper
02 Mar 2020
Regular paper | Highlight paper |  | 02 Mar 2020

On the alignment of velocity and magnetic fields within magnetosheath jets

Ferdinand Plaschke, Maria Jernej, Heli Hietala, and Laura Vuorinen


Interactive discussion

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Status: closed
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AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to minor revisions (review by editor) (30 Dec 2019) by Matina Gkioulidou
AR by Ferdinand Plaschke on behalf of the Authors (31 Dec 2019)  Author's response    Manuscript
ED: Publish as is (26 Jan 2020) by Matina Gkioulidou
Short summary
Jets of solar-wind plasma commonly hit the Earth's magnetosphere. Using data from the four Magnetospheric Multiscale (MMS) spacecraft, we show statistically that within jets the magnetic field is more aligned with the plasma flow direction than outside of these jets. Our study confirms prior simulation results, but it also shows that the average effect is moderate. The jets' magnetic field is important with respect to their impact on space weather.