Ionospheric response to solar extreme ultraviolet radiation variations: comparison based on CTIPe model simulations and satellite measurements

Vaishnav, Rajesh; Schmölter, Erik; Jacobi, Christoph; Berdermann, Jens; Codrescu, Mihail

doi:https://doi.org/10.5194/angeo-39-341-2021

Articles | Volume 39, issue 2

https://doi.org/10.5194/angeo-39-341-2021

© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

https://doi.org/10.5194/angeo-39-341-2021

© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 39, issue 2

Regular paper

|

06 Apr 2021

Regular paper |

| 06 Apr 2021

Ionospheric response to solar extreme ultraviolet radiation variations: comparison based on CTIPe model simulations and satellite measurements

Rajesh Vaishnav, Erik Schmölter, Christoph Jacobi, Jens Berdermann, and Mihail Codrescu

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Final revised paper (published on 06 Apr 2021)
Preprint (discussion started on 11 Dec 2020)

Interactive discussion

Status: closed

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

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- Supplement

RC1: 'Report: angeo-2020-83-manuscript-review', Gerhard Schmidtke, 08 Jan 2021
- AC1: 'Response to Referee #1', RAJESH VAISHNAV, 28 Jan 2021
RC2: 'Review comments for “Ionospheric Response to Solar EUV Radiation Variations: Comparison based on CTIPe Model Simulations and Satellite Measurements” by Vaishnav et al.', Anonymous Referee #2, 10 Jan 2021
- AC2: 'Response to anonymous Referee #2', RAJESH VAISHNAV, 28 Jan 2021

Peer-review completion

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

ED: Publish subject to minor revisions (review by editor) (29 Jan 2021) by Dalia Buresova

AR by RAJESH VAISHNAV on behalf of the Authors (09 Feb 2021) Author's response Author's tracked changes Manuscript

ED: Publish as is (24 Feb 2021) by Dalia Buresova

Short summary

We investigate the delayed ionospheric response using the observed and CTIPe-model-simulated TEC against the solar EUV flux. The ionospheric delay estimated using model-simulated TEC is in good agreement with the delay estimated for observed TEC. The study confirms the model's capabilities to reproduce the delayed ionospheric response against the solar EUV flux. Results also indicate that the average delay is higher in the Northern Hemisphere as compared to the Southern Hemisphere.