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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Series: | Journal of Space Weather and Space Climate |
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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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