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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Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p250_Szajko |
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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 |
work_keys_str_mv |
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_version_ |
1807324553971499008 |