Articles | Volume 37, issue 4
Ann. Geophys., 37, 689–697, 2019
Ann. Geophys., 37, 689–697, 2019

ANGEO Communicates 06 Aug 2019

ANGEO Communicates | 06 Aug 2019

Jets in the magnetosheath: IMF control of where they occur

Laura Vuorinen et al.


Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to technical corrections (02 Jul 2019) by Christopher Mouikis
AR by Laura Vuorinen on behalf of the Authors (12 Jul 2019)  Author's response    Manuscript
Short summary
Before the solar wind encounters the Earth's magnetic field, it is first slowed down and deflected by the Earth's bow shock. We find that downstream of the bow shock regions where the shock normal and the solar wind magnetic field are almost parallel and the shock is more rippled, plasma jets with high earthward velocities are observed significantly more often than elsewhere downstream of the shock. Our results help us forecast the occurrence of these jets and their effects on Earth.