GEOSCAN, résultats de la recherche

Menu GEOSCAN


TitreDevelopment of coronal field and solar wind components for MHD interplanetary simulations
AuteurNikolic, L; Trichtchenko, L
SourceWorld Academy of Science, Engineering and Technology vol. 6, 2012 p. 11-26
LiensOnline - En ligne
Année2012
Séries alt.Secteur des sciences de la Terre, Contribution externe 20120383
RéunionICPP 2012: International Conference on Plasma Physics; Venice; IT; Novembre 14-16, 2012
Documentpublication en série
Lang.anglais
Mediapapier; en ligne; numérique
Formatspdf
Sujetsénergie solaire; variations solaires; géomagnétisme; champs géomagnétiques; variations géomagnétiques; simulations par ordinateur; établissement de modèles; géophysique; géologie extraterrestre
Illustrationsimages; plots
ProgrammeTargeted Hazard Assessments in Northern Canada, Géoscience pour la sécurité publique
Résumé(disponible en anglais seulement)
The connection between solar activity and adverse phenomena in the Earth's environment that can affect space and ground based technologies has spurred interest in the Space Weather (SW) research. Since the most reliable observations, from the L1 point, allow only ~1h advanced warning of approaching solar disturbances, a great effort has been put on the development of suitable models that can provide longer predictions of the SW events. With the progress in computational technology it is possible now to develop operational large scale physics based models which can incorporate most important physical processes and domains of the Sun-Earth system. In order to enhance our SW prediction capabilities we are placing efforts to develop advanced numerical tools. With operational requirements in mind, our goal is to develop a modular simulation framework of propagation of the solar disturbances through interplanetary space. Here, we report and discuss our efforts on the development of coronal field and solar wind components for a large scale MHD code. The model for the components is based on a potential field source surface model and an empirical Wang-Sheeley-Arge solar wind relation.
GEOSCAN ID292200