Articles | Volume 37, issue 6
https://doi.org/10.5194/angeo-37-1141-2019
https://doi.org/10.5194/angeo-37-1141-2019
Regular paper
 | 
10 Dec 2019
Regular paper |  | 10 Dec 2019

Long-term trends in the ionospheric response to solar extreme-ultraviolet variations

Rajesh Vaishnav, Christoph Jacobi, and Jens Berdermann

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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
ED: Reconsider after major revisions (further review by editor and referees) (04 Jul 2019) by Erdal Yiğit
AR by Rajesh Ishwardas Vaishnav on behalf of the Authors (08 Aug 2019)  Author's response   Manuscript 
ED: Referee Nomination & Report Request started (16 Aug 2019) by Erdal Yiğit
RR by Anonymous Referee #1 (23 Aug 2019)
RR by Anonymous Referee #3 (12 Oct 2019)
ED: Publish subject to revisions (further review by editor and referees) (22 Oct 2019) by Erdal Yiğit
AR by Rajesh Ishwardas Vaishnav on behalf of the Authors (25 Oct 2019)  Author's response   Manuscript 
ED: Publish as is (05 Nov 2019) by Erdal Yiğit
AR by Rajesh Ishwardas Vaishnav on behalf of the Authors (08 Nov 2019)
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Short summary
We investigate the ionospheric response to the temporal and spatial dynamics of the solar activity using total electron content (TEC) maps and multiple solar proxies. The maximum correlation at a 16–32-d timescale is observed between the He-II, Mg-II, and F30 with respect to global mean TEC, with an effective time delay of about 1 d. The most suitable proxy to represent the solar activity at the timescales of 16–32 d and 32–64 d is He-II.