Articles | Volume 38, issue 2
https://doi.org/10.5194/angeo-38-287-2020
https://doi.org/10.5194/angeo-38-287-2020
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

Download

Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
Printer-friendly Version - Printer-friendly version Supplement - Supplement

Peer-review completion

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
AR by Ferdinand Plaschke on behalf of the Authors (31 Jan 2020)
Download
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.