Articles | Volume 44, issue 2
https://doi.org/10.5194/angeo-44-949-2026
https://doi.org/10.5194/angeo-44-949-2026
Regular paper
 | 
18 Sep 2026
Regular paper |  | 18 Sep 2026

Deducing spatial characteristics of global thunderstorm activity using the observed Schumann resonance frequencies

Oleksandr Koloskov, Masashi Hayakawa, and Alexander P. Nickolaenko

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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 egusphere-2025-5961', Anonymous Referee #1, 22 Jan 2026
    • RC2: 'Reply on RC1', Anonymous Referee #2, 27 Mar 2026
      • AC2: 'Reply on RC2', Oleksandr Koloskov, 10 May 2026
    • AC1: 'Reply on RC1', Oleksandr Koloskov, 10 May 2026

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) (21 May 2026) by Dalia Buresova
AR by Oleksandr Koloskov on behalf of the Authors (24 May 2026)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (26 May 2026) by Dalia Buresova
RR by Anonymous Referee #1 (16 Jun 2026)
ED: Reconsider after major revisions (further review by editor and referees) (10 Jul 2026) by Dalia Buresova
AR by Oleksandr Koloskov on behalf of the Authors (24 Jul 2026)  Author's response   Author's tracked changes   Manuscript 
ED: Referee Nomination & Report Request started (12 Aug 2026) by Dalia Buresova
RR by Anonymous Referee #1 (14 Aug 2026)
ED: Publish as is (17 Aug 2026) by Dalia Buresova
AR by Oleksandr Koloskov on behalf of the Authors (24 Aug 2026)  Manuscript 
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Short summary
To study global thunderstorm activity we analysed the Schumann Resonance electromagnetic field driven by lightning. We developed formulas to calculate both the distance and the size of thunderstorm areas from frequency changes of either the magnetic or the electric resonance modes alone. Our method can be used by observatories worldwide, which mainly record magnetic fields. This novel technique improves our ability to monitor and understand global lightning activity.
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