A Carrington-like geomagnetic storm observed in the 21st century

In September 1859 the Colaba observatory measured the most extreme geomagnetic disturbance ever recorded at low latitudes related to solar activity: the Carrington storm. This paper describes a geomagnetic disturbance case with a profile extraordinarily similar to the disturbance of the Carrington e...

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Main Authors: Cid Consuelo, Saiz Elena, Guerrero Antonio, Palacios Judith, Cerrato Yolanda
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:Journal of Space Weather and Space Climate
Online Access:http://dx.doi.org/10.1051/swsc/2015017
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spelling doaj-0a794f1889184b93bd3397f2f715a4aa2021-04-02T09:52:27ZengEDP SciencesJournal of Space Weather and Space Climate2115-72512015-01-015A1610.1051/swsc/2015017swsc140015A Carrington-like geomagnetic storm observed in the 21st centuryCid ConsueloSaiz ElenaGuerrero AntonioPalacios JudithCerrato YolandaIn September 1859 the Colaba observatory measured the most extreme geomagnetic disturbance ever recorded at low latitudes related to solar activity: the Carrington storm. This paper describes a geomagnetic disturbance case with a profile extraordinarily similar to the disturbance of the Carrington event at Colaba: the event on 29 October 2003 at Tihany magnetic observatory in Hungary. The analysis of the H-field at different locations during the “Carrington-like” event leads to a re-interpretation of the 1859 event. The major conclusions of the paper are the following: (a) the global Dst or SYM-H, as indices based on averaging, missed the largest geomagnetic disturbance in the 29 October 2003 event and might have missed the 1859 disturbance, since the large spike in the horizontal component (H) of terrestrial magnetic field depends strongly on magnetic local time (MLT); (b) the main cause of the large drop in H recorded at Colaba during the Carrington storm was not the ring current but field-aligned currents (FACs); and (c) the very local signatures of the H-spike imply that a Carrington-like event can occur more often than expected.http://dx.doi.org/10.1051/swsc/2015017
collection DOAJ
language English
format Article
sources DOAJ
author Cid Consuelo
Saiz Elena
Guerrero Antonio
Palacios Judith
Cerrato Yolanda
spellingShingle Cid Consuelo
Saiz Elena
Guerrero Antonio
Palacios Judith
Cerrato Yolanda
A Carrington-like geomagnetic storm observed in the 21st century
Journal of Space Weather and Space Climate
author_facet Cid Consuelo
Saiz Elena
Guerrero Antonio
Palacios Judith
Cerrato Yolanda
author_sort Cid Consuelo
title A Carrington-like geomagnetic storm observed in the 21st century
title_short A Carrington-like geomagnetic storm observed in the 21st century
title_full A Carrington-like geomagnetic storm observed in the 21st century
title_fullStr A Carrington-like geomagnetic storm observed in the 21st century
title_full_unstemmed A Carrington-like geomagnetic storm observed in the 21st century
title_sort carrington-like geomagnetic storm observed in the 21st century
publisher EDP Sciences
series Journal of Space Weather and Space Climate
issn 2115-7251
publishDate 2015-01-01
description In September 1859 the Colaba observatory measured the most extreme geomagnetic disturbance ever recorded at low latitudes related to solar activity: the Carrington storm. This paper describes a geomagnetic disturbance case with a profile extraordinarily similar to the disturbance of the Carrington event at Colaba: the event on 29 October 2003 at Tihany magnetic observatory in Hungary. The analysis of the H-field at different locations during the “Carrington-like” event leads to a re-interpretation of the 1859 event. The major conclusions of the paper are the following: (a) the global Dst or SYM-H, as indices based on averaging, missed the largest geomagnetic disturbance in the 29 October 2003 event and might have missed the 1859 disturbance, since the large spike in the horizontal component (H) of terrestrial magnetic field depends strongly on magnetic local time (MLT); (b) the main cause of the large drop in H recorded at Colaba during the Carrington storm was not the ring current but field-aligned currents (FACs); and (c) the very local signatures of the H-spike imply that a Carrington-like event can occur more often than expected.
url http://dx.doi.org/10.1051/swsc/2015017
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