Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution

We revisit previous studies in which the characteristics of the solar and interplanetary sources of intense geomagnetic storms have been discussed. We consider the very intense geomagnetic storms that occurred during Solar Cycle 23 by setting a value of Dst min <-200 nT as threshold. We have...

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Autores principales: Szajko, N., Cristiani, G., Dal Lago, A., Mandrini, C.H., Mandrini C.H., Webb D.F.
Formato: SER
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p250_Szajko
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spelling todo:paper_17439213_v7_nS286_p250_Szajko2023-10-03T16:31:40Z Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution Szajko, N. Cristiani, G. Dal Lago, A. Mandrini, C.H. Mandrini C.H. Webb D.F. interplanetary medium Sun: activity Sun: coronal mass ejections (CMEs) We revisit previous studies in which the characteristics of the solar and interplanetary sources of intense geomagnetic storms have been discussed. We consider the very intense geomagnetic storms that occurred during Solar Cycle 23 by setting a value of Dst min <-200 nT as threshold. We have identified and characterized the solar and interplanetary sources of each storm. After this, we investigate the overall characteristics of the interplanetary (IP) main-phase storm driver, including the time arrival of the shock/disturbance at 1 AU, the type of associated IP structure/ejecta, the origin of a prolonged and enhanced southward component (B z) of the IP field, and other characteristics related to the energy injected into the magnetosphere during the storm. © 2012 International Astronomical Union. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p250_Szajko
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic interplanetary medium
Sun: activity
Sun: coronal mass ejections (CMEs)
spellingShingle interplanetary medium
Sun: activity
Sun: coronal mass ejections (CMEs)
Szajko, N.
Cristiani, G.
Dal Lago, A.
Mandrini, C.H.
Mandrini C.H.
Webb D.F.
Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution
topic_facet interplanetary medium
Sun: activity
Sun: coronal mass ejections (CMEs)
description We revisit previous studies in which the characteristics of the solar and interplanetary sources of intense geomagnetic storms have been discussed. We consider the very intense geomagnetic storms that occurred during Solar Cycle 23 by setting a value of Dst min <-200 nT as threshold. We have identified and characterized the solar and interplanetary sources of each storm. After this, we investigate the overall characteristics of the interplanetary (IP) main-phase storm driver, including the time arrival of the shock/disturbance at 1 AU, the type of associated IP structure/ejecta, the origin of a prolonged and enhanced southward component (B z) of the IP field, and other characteristics related to the energy injected into the magnetosphere during the storm. © 2012 International Astronomical Union.
format SER
author Szajko, N.
Cristiani, G.
Dal Lago, A.
Mandrini, C.H.
Mandrini C.H.
Webb D.F.
author_facet Szajko, N.
Cristiani, G.
Dal Lago, A.
Mandrini, C.H.
Mandrini C.H.
Webb D.F.
author_sort Szajko, N.
title Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution
title_short Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution
title_full Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution
title_fullStr Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution
title_full_unstemmed Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution
title_sort very intense geomagnetic storms: solar sources, characteristics and cycle distribution
url http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p250_Szajko
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AT cristianig veryintensegeomagneticstormssolarsourcescharacteristicsandcycledistribution
AT dallagoa veryintensegeomagneticstormssolarsourcescharacteristicsandcycledistribution
AT mandrinich veryintensegeomagneticstormssolarsourcescharacteristicsandcycledistribution
AT mandrinich veryintensegeomagneticstormssolarsourcescharacteristicsandcycledistribution
AT webbdf veryintensegeomagneticstormssolarsourcescharacteristicsandcycledistribution
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