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...

Descripción completa

Guardado en:

Detalles Bibliográficos
Autores principales:	Szajko, N., Cristiani, G., Dal Lago, A., Mandrini, C.H., Mandrini C.H., Webb D.F.
Formato:	SER
Materias:	interplanetary medium Sun: activity Sun: coronal mass ejections (CMEs)
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_17439213_v7_nS286_p250_Szajko
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Very intense geomagnetic storms: Solar sources, characteristics and cycle distribution
Publicado: (2011)

Flux rope axis geometry of magnetic clouds deduced from in situ data
Publicado: (2013)

Flux rope axis geometry of magnetic clouds deduced from in situ data
por: Janvier, M., et al.

Coronal transients during two solar minima: Their source regions and interplanetary counterparts
por: Cremades, H., et al.
Publicado: (2011)

Coronal transients during two solar minima: Their source regions and interplanetary counterparts
por: Cremades, H., et al.

Coronal transients during two solar minima: Their source regions and interplanetary counterparts
por: Cremades, H., et al.
Publicado: (2011)

A new model-independent method to compute magnetic helicity in magnetic clouds
por: Dasso, S., et al.
Publicado: (2006)

A new model-independent method to compute magnetic helicity in magnetic clouds
por: Dasso, S., et al.

A new model-independent method to compute magnetic helicity in magnetic clouds
por: Dasso, S., et al.
Publicado: (2006)

An eruptive complex solar flare and events in its aftermath
por: Luoni, M.L., et al.

SOHO/ACE observations of two consecutive CMEs from the same source region
por: Schettino, G., et al.
Publicado: (2010)

SOHO/ACE observations of two consecutive CMEs from the same source region
por: Schettino, G., et al.

SOHO/ACE observations of two consecutive CMEs from the same source region
por: Schettino, G., et al.
Publicado: (2010)

A long-duration active region: Evolution and quadrature observations of ejective events
por: Cremades, H., et al.

Clarifying some issues on the geoeffectiveness of limb halo CMEs
por: Mandrini, Cristina Hemilse, et al.
Publicado: (2013)

A new model-independent method to compute magnetic helicity in magnetic clouds
por: Dasso, Sergio Ricardo, et al.
Publicado: (2006)

Coronal transients during two solar minima: Their source regions and interplanetary counterparts
por: Mandrini, Cristina Hemilse, et al.
Publicado: (2011)

SOHO/ACE observations of two consecutive CMEs from the same source region
por: Dasso, Sergio Ricardo, et al.
Publicado: (2010)

Observational consequences of a magnetic flux rope emerging into the corona
por: Gibson, S.E., et al.

Clarifying some issues on the geoeffectiveness of limb halo CMEs
por: Cid, C., et al.
Publicado: (2013)

Clarifying some issues on the geoeffectiveness of limb halo CMEs
por: Cid, C., et al.

Clarifying some issues on the geoeffectiveness of limb halo CMEs
por: Cid, C., et al.
Publicado: (2013)

Evolution of spinning and braiding helicity fluxes in solar active region NOAA 10930
por: Dasso, Sergio Ricardo
Publicado: (2011)

Evolution of spinning and braiding helicity fluxes in solar active region NOAA 10930
por: Ravindra, B., et al.
Publicado: (2011)

Evolution of spinning and braiding helicity fluxes in solar active region NOAA 10930
por: Ravindra, B., et al.

Evolution of spinning and braiding helicity fluxes in solar active region NOAA 10930
por: Ravindra, B., et al.
Publicado: (2011)

Magnetic energy release and topology in solar active phenomena
por: Mandrini, Cristina Hemilse
Publicado: (2019)

Magnetic helicity budget of solar-active regions from the photosphere to magnetic clouds
por: Mandrini, C.H., et al.

Análisis de la evolución de una eyección coronal de masa del tipo Streamer Blowout
por: Di Lorenzo, L., et al.
Publicado: (2023)

Expansión y autosimilitud de eyecciones coronales de masa a partir de observaciones estereoscópicas
por: Cremades, H., et al.
Publicado: (2019)

An eruptive complex solar flare and events in its aftermath
Publicado: (2016)

A long-duration active region: Evolution and quadrature observations of ejective events
Publicado: (2016)

Configuración magnética preeruptiva de la región NOAA 12127 mediante extrapolación no lineal del campo
por: Merenda, L. A., et al.
Publicado: (2021)

Observational consequences of a magnetic flux rope emerging into the corona
Publicado: (2004)

Expansión de eyecciones coronales de masa y ondas de choque en la corona solar
por: Balmaceda, Laura Antonia
Publicado: (2022)

Very intense geomagnetic storms and their relation to interplanetary and solar active phenomena
por: Szajko, N.S., et al.

Galactic cosmic ray decreases associated with non-interacting magnetic clouds in the 23rd solar cycle
por: Dasso, Sergio Ricardo
Publicado: (2013)

Galactic cosmic ray decreases associated with non-interacting magnetic clouds in the 23rd solar cycle
por: Masías-Meza, J.J., et al.
Publicado: (2013)

Galactic cosmic ray decreases associated with non-interacting magnetic clouds in the 23rd solar cycle
por: Masías-Meza, J.J., et al.

Galactic cosmic ray decreases associated with non-interacting magnetic clouds in the 23rd solar cycle
por: Masías-Meza, J.J., et al.
Publicado: (2013)