Articles | Volume 28, issue 2
Nonlin. Processes Geophys., 28, 257–270, 2021
https://doi.org/10.5194/npg-28-257-2021
Nonlin. Processes Geophys., 28, 257–270, 2021
https://doi.org/10.5194/npg-28-257-2021

Research article 19 May 2021

Research article | 19 May 2021

Magnetospheric chaos and dynamical complexity response during storm time disturbance

Irewola Aaron Oludehinwa et al.

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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
AR by Oludehinwa Irewola on behalf of the Authors (05 Mar 2021)  Author's response    Author's tracked changes    Manuscript
ED: Referee Nomination & Report Request started (06 Mar 2021) by Giovanni Lapenta
RR by Bruce Tsurutani (06 Mar 2021)
RR by Anonymous Referee #2 (16 Mar 2021)
ED: Reconsider after major revisions (further review by editor and referees) (16 Mar 2021) by Giovanni Lapenta
AR by Oludehinwa Irewola on behalf of the Authors (26 Mar 2021)  Author's response    Author's tracked changes    Manuscript
ED: Referee Nomination & Report Request started (06 Apr 2021) by Giovanni Lapenta
RR by Anonymous Referee #1 (06 Apr 2021)
ED: Publish subject to minor revisions (review by editor) (07 Apr 2021) by Giovanni Lapenta
AR by Oludehinwa Irewola on behalf of the Authors (08 Apr 2021)  Author's response    Author's tracked changes    Manuscript
ED: Publish as is (16 Apr 2021) by Giovanni Lapenta
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Short summary
The MLE and ApEn values of the Dst indicate that chaotic and dynamical complexity responses are high during minor geomagnetic storms, reduce at moderate geomagnetic storms and decline further during major geomagnetic storms. However, the MLE and ApEn values obtained from solar wind electric field (VBs) indicate that chaotic and dynamical complexity responses are high with no significant difference between the periods that are associated with minor, moderate and major geomagnetic storms.