Articles | Volume 39, issue 3
https://doi.org/10.5194/angeo-39-379-2021
https://doi.org/10.5194/angeo-39-379-2021
Regular paper
 | 
05 May 2021
Regular paper |  | 05 May 2021

Warm protons at comet 67P/Churyumov–Gerasimenko – implications for the infant bow shock

Charlotte Goetz, Herbert Gunell, Fredrik Johansson, Kristie LLera, Hans Nilsson, Karl-Heinz Glassmeier, and Matthew G. G. T. Taylor

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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 revisions (further review by editor and referees) (10 Mar 2021) by Elias Roussos
AR by Charlotte Götz on behalf of the Authors (11 Mar 2021)  Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (16 Mar 2021) by Elias Roussos
RR by Anonymous Referee #1 (18 Mar 2021)
ED: Publish as is (18 Mar 2021) by Elias Roussos
AR by Charlotte Götz on behalf of the Authors (24 Mar 2021)
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Short summary
Boundaries in the plasma around comet 67P separate regions with different properties. Many have been identified, including a new boundary called an infant bow shock. Here, we investigate how the plasma and fields behave at this boundary and where it can be found. The main result is that the infant bow shock occurs at intermediate activity and intermediate distances to the comet. Most plasma parameters behave as expected; however, some inconsistencies indicate that the boundary is non-stationary.