High-latitude crochet: solar-flare-induced magnetic disturbance independent from low-latitude crochet

Yamauchi, Masatoshi; Johnsen, Magnar G.; Enell, Carl-Fredrik; Tjulin, Anders; Willer, Anna; Sormakov, Dmitry A.

doi:https://doi.org/10.5194/angeo-38-1159-2020

Articles | Volume 38, issue 6

https://doi.org/10.5194/angeo-38-1159-2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

https://doi.org/10.5194/angeo-38-1159-2020

© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Articles | Volume 38, issue 6

Regular paper

|

03 Nov 2020

Regular paper |

| 03 Nov 2020

High-latitude crochet: solar-flare-induced magnetic disturbance independent from low-latitude crochet

Masatoshi Yamauchi, Magnar G. Johnsen, Carl-Fredrik Enell, Anders Tjulin, Anna Willer, and Dmitry A. Sormakov

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Final revised paper (published on 03 Nov 2020)
Supplement to the final revised paper
Preprint (discussion started on 09 Jul 2020)

Interactive discussion

Status: closed

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

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- Supplement

RC1: 'angeo-2020-48 _ Comments_ High-latitude crochet: solar flare-induced magnetic disturbance independent from low-latitude', Anonymous Referee #1, 04 Aug 2020
- AC1: 'Authors' reply to Referee #1', Masatoshi Yamauchi, 11 Aug 2020
RC2: 'Review on "High-latitude crochet: solar flare-induced magnetic disturbance independent from low-latitude" by Yamauchi et al.', Anonymous Referee #2, 18 Aug 2020
- AC2: 'Reply to Referee #2', Masatoshi Yamauchi, 22 Aug 2020

Peer-review completion

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

ED: Publish subject to minor revisions (review by editor) (25 Aug 2020) by Dalia Buresova

AR by Masatoshi Yamauchi on behalf of the Authors (29 Aug 2020) Author's response Manuscript

ED: Publish as is (07 Sep 2020) by Dalia Buresova

Short summary

The paper reports a new finding on space weather effects at around 70–75 ° geographic latitudes. We found that X flares cause an unexpectedly strong ionospheric current driven by solar flares. The effect is as large as a substorm that is known to cause strong auroras and may enhance ongoing substorms. However, it has been overlooked in the past due to the narrow latitudinal range at high latitudes. Since severe magnetic storms often occur with X flares, this may cause geomagnetic hazards.