Wavelet analysis of the magnetotail response to solar wind fluctuations during HILDCAA events

Marques de Souza Franco, Adriane; Echer, Ezequiel; José Alves Bolzan, Mauricio

doi:https://doi.org/10.5194/angeo-37-919-2019

Articles | Volume 37, issue 5

https://doi.org/10.5194/angeo-37-919-2019

© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

Special issue:

7th Brazilian meeting on space geophysics and aeronomy

https://doi.org/10.5194/angeo-37-919-2019

© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 37, issue 5

Regular paper

|

09 Oct 2019

Regular paper |

| 09 Oct 2019

Wavelet analysis of the magnetotail response to solar wind fluctuations during HILDCAA events

Adriane Marques de Souza Franco, Ezequiel Echer, and Mauricio José Alves Bolzan

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Final revised paper (published on 09 Oct 2019)
Preprint (discussion started on 20 May 2019)

Interactive discussion

Status: closed

AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment

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- Supplement

RC1: 'Comments on “Wavelet analysis of the magnetotail response to solar wind fluctuations during HILDCCA events” by A. M. S. Franco, E. Echer, and M. J. A. Bolzan', Rajkumar Hajra, 10 Jun 2019
- AC1: 'reply to the referee', Adriane Marques de Souza Franco, 24 Jun 2019
EC1: 'Revision needed', Inez Batista, 10 Jun 2019
RC2: 'Review', Anonymous Referee #2, 26 Jun 2019
- AC2: 'Response to Reviewer 2', Adriane Marques de Souza Franco, 28 Jun 2019

Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision

ED: Publish subject to revisions (further review by editor and referees) (01 Aug 2019) by Inez Batista

AR by Adriane Marques de Souza Franco on behalf of the Authors (02 Aug 2019) Author's response Manuscript

ED: Referee Nomination & Report Request started (05 Aug 2019) by Inez Batista

RR by Anonymous Referee #2 (13 Aug 2019)

RR by Rajkumar Hajra (30 Aug 2019)

ED: Publish as is (03 Sep 2019) by Inez Batista

AR by Adriane Marques de Souza Franco on behalf of the Authors (06 Sep 2019)

Short summary

The wavelet transform was employed in nine HILDCAA events for intervals in which the Cluster crossed the magnetotail in order to identify the most energetic periods of these events in the magnetotail. It was seen that 76 % of the periods identified are ≤4 h. Using the cross wavelet analysis technique between B_z–IMF components and the B_x geomagnetic components, it was identified that the coupling of energy is stronger in periods between 2 and 4 h, which are typical substorm periods.