Articles | Volume 40, issue 5
Ann. Geophys., 40, 585–603, 2022
https://doi.org/10.5194/angeo-40-585-2022
Ann. Geophys., 40, 585–603, 2022
https://doi.org/10.5194/angeo-40-585-2022
Regular paper
06 Oct 2022
Regular paper | 06 Oct 2022

Ionospheric effects of the 5–6 January 2019 eclipse over the People's Republic of China: results from oblique sounding

Leonid F. Chernogor et al.

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Interactive discussion

Status: closed

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on angeo-2022-15', Anonymous Referee #1, 10 Jun 2022
    • AC1: 'Reply on RC1', Yu Zheng, 05 Jul 2022
  • RC2: 'Comment on angeo-2022-15', Anonymous Referee #2, 30 Jun 2022
    • AC2: 'Reply on RC2', Yu Zheng, 06 Jul 2022

Peer review completion

AR: Author's response | RR: Referee report | ED: Editor decision
ED: Reconsider after major revisions (further review by editor and referees) (07 Jul 2022) by Ana G. Elias
AR by Yu Zheng on behalf of the Authors (07 Jul 2022)  Author's response    Author's tracked changes    Manuscript
ED: Referee Nomination & Report Request started (11 Jul 2022) by Ana G. Elias
RR by Anonymous Referee #2 (22 Aug 2022)
ED: Publish as is (29 Aug 2022) by Ana G. Elias
AR by Yu Zheng on behalf of the Authors (30 Aug 2022)  Author's response
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Short summary
The solar eclipse of 5–6 January 2019 perturbed the ionospheric electron density, N, observed with the receiver at the Harbin Engineering University and 14 HF broadcasting stations ~1 000 km around. It was accompanied by ±1.5 Hz Doppler-spectrum broadening, ±0.5 Hz Doppler shift, fD, variations, 15 min period variations in fD caused by 1.6–2.4 % perturbations in N, and period changes of 4–5 min in fD caused by 0.2–0.3 % disturbances in N. The decrease in N attained ~15 % (vs. modeled 16 %).