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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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ANGEO | Articles | Volume 36, issue 6
Ann. Geophys., 36, 1537-1543, 2018
https://doi.org/10.5194/angeo-36-1537-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 36, 1537-1543, 2018
https://doi.org/10.5194/angeo-36-1537-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.

ANGEO Communicates 15 Nov 2018

ANGEO Communicates | 15 Nov 2018

Can an interplanetary magnetic field reach the surface of Venus?

Yasuhito Narita and Uwe Motschmann
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Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to revisions (further review by editor and referees) (04 Oct 2018) by Elias Roussos
AR by Yasuhito Narita on behalf of the Authors (04 Oct 2018)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (06 Oct 2018) by Elias Roussos
RR by Anonymous Referee #1 (24 Oct 2018)
ED: Publish subject to minor revisions (review by editor) (26 Oct 2018) by Elias Roussos
AR by Yasuhito Narita on behalf of the Authors (01 Nov 2018)  Author's response    Manuscript
ED: Publish as is (06 Nov 2018) by Elias Roussos
Publications Copernicus
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Short summary
Venus has no intrinsic magnetic field. On the other hand, we discover that an interplanetary magnetic field may nevertheless penetrate the planetary ionosphere by the diffusion process and reach the planetary surface when the solar wind condition remains for a sufficiently long time, between 12 and 54 h, depending on the condition of ionosphere.
Venus has no intrinsic magnetic field. On the other hand, we discover that an interplanetary...
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