Articles | Volume 38, issue 1
Ann. Geophys., 38, 51–60, 2020
Ann. Geophys., 38, 51–60, 2020

Regular paper 15 Jan 2020

Regular paper | 15 Jan 2020

On the magnetic characteristics of magnetic holes in the solar wind between Mercury and Venus

Martin Volwerk 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 minor revisions (review by editor) (22 Nov 2019) by Anna Milillo
AR by Martin Volwerk on behalf of the Authors (22 Nov 2019)  Author's response    Manuscript
ED: Publish subject to technical corrections (11 Dec 2019) by Anna Milillo
Short summary
The magnetic field that is carried by the solar wind slowly decreases in strength as it moves further from the Sun. However, there are sometimes localized decreases in the magnetic field strength, called magnetic holes. These are small structures where the magnetic field strength decreases to less than 50 % of the surroundings and the plasma density increases. This paper presents a statistical study of the behaviour of these holes between Mercury and Venus using MESSENGER data.