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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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ANGEO | Articles | Volume 38, issue 5
Ann. Geophys., 38, 953–968, 2020
https://doi.org/10.5194/angeo-38-953-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
Ann. Geophys., 38, 953–968, 2020
https://doi.org/10.5194/angeo-38-953-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Regular paper 04 Sep 2020

Regular paper | 04 Sep 2020

Semiannual variation of Pc5 ultra-low frequency (ULF) waves and relativistic electrons over two solar cycles of observations: comparison with predictions of the classical hypotheses

Facundo L. Poblet et al.

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Status: closed
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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) (05 May 2020) by Vincent Maget
AR by Facundo Poblet on behalf of the Authors (20 May 2020)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (26 May 2020) by Vincent Maget
RR by Anonymous Referee #2 (26 May 2020)
RR by Anonymous Referee #1 (19 Jul 2020)
ED: Publish subject to technical corrections (20 Jul 2020) by Vincent Maget
AR by Facundo Poblet on behalf of the Authors (30 Jul 2020)  Author's response    Manuscript
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Short summary
High-energy electrons in the magnetosphere can cause operational anomalies in satellites. We investigate regular variations in these electrons and in Pc5 low-frequency waves that are capable of generating the energetic electrons. We find that both variables present similar periods in every solar cycle phase. We focus the analysis on the semiannual variation of these parameters. The shape of the observational semiannual curves correlate very well with the profiles of the main theories.
High-energy electrons in the magnetosphere can cause operational anomalies in satellites. We...
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