Codi QR

Cosmic ray intensity during the passage of coronal mass ejections

Coronal Mass Ejections are vast structures of plasma and magnetic fields that are expelled from the sun into the heliosphere. This material is detected by remote sensing and in-situ spacecraft observations. The present study deals with the influence of four types of CMEs namely Asymmetric 'Full' Hal...

Descripció completa

Guardat en:
Dades bibliogràfiques
Publicat a:Brazilian Journal of Physics
Autors principals: Rajesh K. Mishra, Rekha Agarwal
Format: Artigo
Idioma:Inglês
Publicat: Sociedade Brasileira de Física 2008
Matèries:
Accés en línia:https://www.redalyc.org/articulo.oa?id=46413554007
Etiquetes: Afegir etiqueta
Sense etiquetes, Sigues el primer a etiquetar aquest registre!