The forecasting of intense geomagnetic storms

Intense geomagnetic storms are produced by the arrival at the magnetopause of solar wind carrying a magnetic field with a large southward component lasting for several hours. Solar and interplanetary processes have been considered to explain the presence of this field, but many aspects of its origin...

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Main Author: Silvia Bravo
Format: Article
Language:English
Published: Universidad Nacional Autónoma de México, Instituto de Geofísica 1997-04-01
Series:Geofísica Internacional
Subjects:
Online Access:http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/1997/02/bravo.html
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author Silvia Bravo
author_facet Silvia Bravo
author_sort Silvia Bravo
collection DOAJ
description Intense geomagnetic storms are produced by the arrival at the magnetopause of solar wind carrying a magnetic field with a large southward component lasting for several hours. Solar and interplanetary processes have been considered to explain the presence of this field, but many aspects of its origin are still unclear. The general problem of forecasting intense geo¬magnetic storms several days in advance from solar observations is discussed, reviewing the different approaches taken so far and extending a previous study of the solar sources of major geomagnetic storms. All evidence favours the occurrence of an explosive event (flare or prominence eruption) near a coronal hole and near the solar central meridian as a potentially geoeffective solar event. Comments are made on how our forecasting capability may improve with the use of soft X-ray im¬ages of coronal transients, numerical MHD simulations of the generation and propagation of solar transients in the inter¬planetary medium, and tracking of solar wind disturbances by means of interplanetary scintillation.
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spelling doaj.art-a7a8273d11a24c0589c2e969d7d3623f2023-09-03T06:51:41ZengUniversidad Nacional Autónoma de México, Instituto de GeofísicaGeofísica Internacional0016-71691997-04-01362127135The forecasting of intense geomagnetic stormsSilvia BravoIntense geomagnetic storms are produced by the arrival at the magnetopause of solar wind carrying a magnetic field with a large southward component lasting for several hours. Solar and interplanetary processes have been considered to explain the presence of this field, but many aspects of its origin are still unclear. The general problem of forecasting intense geo¬magnetic storms several days in advance from solar observations is discussed, reviewing the different approaches taken so far and extending a previous study of the solar sources of major geomagnetic storms. All evidence favours the occurrence of an explosive event (flare or prominence eruption) near a coronal hole and near the solar central meridian as a potentially geoeffective solar event. Comments are made on how our forecasting capability may improve with the use of soft X-ray im¬ages of coronal transients, numerical MHD simulations of the generation and propagation of solar transients in the inter¬planetary medium, and tracking of solar wind disturbances by means of interplanetary scintillation.http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/1997/02/bravo.htmlGeomagnetic stormsinterplanetary disturbancessolar activity
spellingShingle Silvia Bravo
The forecasting of intense geomagnetic storms
Geofísica Internacional
Geomagnetic storms
interplanetary disturbances
solar activity
title The forecasting of intense geomagnetic storms
title_full The forecasting of intense geomagnetic storms
title_fullStr The forecasting of intense geomagnetic storms
title_full_unstemmed The forecasting of intense geomagnetic storms
title_short The forecasting of intense geomagnetic storms
title_sort forecasting of intense geomagnetic storms
topic Geomagnetic storms
interplanetary disturbances
solar activity
url http://www.geofisica.unam.mx/unid_apoyo/editorial/publicaciones/investigacion/geofisica_internacional/anteriores/1997/02/bravo.html
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