A Carrington-like geomagnetic storm observed in the 21st century
Authors
Cid Tortuero, ConsueloIdentifiers
Permanent link (URI): http://hdl.handle.net/10017/29324DOI: 10.1051/swsc/2015017
ISSN: 2115-7251
Date
2015-05-21Funders
Ministerio de Economía, Industria y Competitividad
Junta de Comunidades de Castilla-La Mancha
Bibliographic citation
Journal of Space Weather and Space Climate, 2015, v. A16, n. 5, p. 1-6
Keywords
Geomagnetics storms
Space Physics
Solar and Stellar Astrophysics
Project
AYA2013-47735-P (Ministerio de Economía, Industria y Competitividad)
PPII10-0183-7802(Junta de Comunidades de Castilla-La Mancha)
PPII10-0183-7802(Junta de Comunidades de Castilla-La Mancha)
Document type
info:eu-repo/semantics/article
Version
info:eu-repo/semantics/publishedVersion
Publisher's version
http:/7dx.doi.org/10.1051/swsc/2015017Rights
Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)© EDP Sciences, 2015
© EDP Sciences, 2015
Access rights
info:eu-repo/semantics/openAccess
Abstract
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.
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Saiz_Journal_of_space_2015.pdf | 342.8Kb |
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