Correction: Earth Planets Space 74:88 (2022) https://doi.org/10.1186/s40623-022-01637-y
Following publication of the original article (Sobhkhiz-Miandehi et al. 2022), the authors found errors in Figs. 5, 6, 7, and 8.
In the originally published PDF, there were errors in VIC calculation process. Thus, we have re-calculated VIC and updated the relevant figures. According to the new Fig. 5, the seasonal variation of DW1 component of EsOR 20 at 110±5km is best correlated to that of VIC at 110km rather than EsOR and VIC at other altitudes. Their correlation coefficient is 0.89, although it can decrease to as low as 0.2 at 100 km altitude. We note that in general a tidal component of EsOR tends to have the highest correlation with the same tidal component of VIC at altitudes higher than 105 km.
The correct Fig. 5 should be:
The correct Fig. 6 should be:
The correct Fig. 7 should be:
The correct Fig. 8 should be:
The original article (Sobhkhiz-Miandehi et al. 2022) has been updated.
Reference
Sobhkhiz-Miandehi S, Yamazaki Y, Arras C, Miyoshi Y, Shinagawa H (2022) Comparison of the tidal signatures in sporadic E and vertical ion convergence rate, using FORMOSAT-3/COSMIC radio occultation observations and GAIA model. Earth Planets Space 74:88. https://doi.org/10.1186/s40623-022-01637-y
Author information
Authors and Affiliations
Corresponding author
Additional information
Publisher's Note
Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Rights and permissions
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/.
About this article
Cite this article
Sobhkhiz‑Miandehi, S., Yamazaki, Y., Arras, C. et al. Correction: Comparison of the tidal signatures in sporadic E and vertical ion convergence rate, using FORMOSAT-3/COSMIC radio occultation observations and GAIA model. Earth Planets Space 75, 160 (2023). https://doi.org/10.1186/s40623-023-01906-4
Published:
DOI: https://doi.org/10.1186/s40623-023-01906-4