| Issue |
J. Space Weather Space Clim.
Volume 10, 2020
Topical Issue - Scientific Advances from the European Commission H2020 projects on Space Weather
|
|
|---|---|---|
| Article Number | 16 | |
| Number of page(s) | 5 | |
| DOI | https://doi.org/10.1051/swsc/2020016 | |
| Published online | 20 April 2020 | |
Reply on Comment
Answer to the comments on “Confirming geomagnetic Sfe by means of a solar flare detector based on GNSS”
1
Observatorio del Ebro, (OE) CSIC – Universitat Ramon Llull (URL), 43520 Roquetes, Spain
2
Research group on Astronomy and Geomatics (gAGE), Universitat Politècnica de Catalunya (UPC), Jordi Girona, 1–3, 08034 Barcelona, Spain
* Corresponding author: jjcurto@obsebre.es
Received:
7
February
2020
Accepted:
11
March
2020
Hernández-Pajares and García-Rigo have written a document criticizing our paper “Confirming geomagnetic Sfe by means of a solar flare detector based on GNSS. J Space Weather Space Clim 9: A42. https://doi.org/10.1051/swsc/2019040” (Curto et al., 2019). The main goal of our paper was to define a methodology based on GNSS measurements that is able to detect solar flares (SF) in an automatic way. This methodology was used to confirm Sfe (SF effects) detected by geomagnetism in an unsupervised manner. In their document, Hernández-Pajares and García-Rigo posed two objections related to the correctness and the novelty of the methodology used in our paper. This document is a reply to these objections and concludes that they are not relevant.
Key words: Sfe detection / GNSS-SF / rise time / solar flares / ionospheric disturbances
© J.J. Curto et al., Published by EDP Sciences 2020
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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