Articles | Volume 41, issue 1
https://doi.org/10.5194/angeo-41-253-2023
https://doi.org/10.5194/angeo-41-253-2023
Regular paper
 | 
31 May 2023
Regular paper |  | 31 May 2023

Concerning the detection of electromagnetic knot structures in space plasmas using the wave telescope technique

Simon Toepfer, Karl-Heinz Glassmeier, and Uwe Motschmann

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Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on angeo-2023-4', Anonymous Referee #1, 12 Apr 2023
    • AC1: 'Reply on RC1', Simon Töpfer, 19 Apr 2023
  • RC2: 'Comment on angeo-2023-4', Anonymous Referee #2, 12 Apr 2023
    • AC2: 'Reply on RC2', Simon Töpfer, 19 Apr 2023

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
ED: Publish subject to revisions (further review by editor and referees) (24 Apr 2023) by Elena Kronberg
AR by Simon Töpfer on behalf of the Authors (02 May 2023)  Author's response   Author's tracked changes   Manuscript 
ED: Publish as is (06 May 2023) by Elena Kronberg
AR by Simon Töpfer on behalf of the Authors (08 May 2023)  Author's response   Manuscript 
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Short summary
The present study discusses the modeling and interpretation of magnetospheric structures via electromagnetic knots for the first time. The mathematical foundations of electromagnetic knots are presented, and the formalism is reformulated in terms of the classical wave telescope technique. The method is tested against synthetically generated magnetic field data describing a plasmoid as a two-dimensional magnetic ring structure.