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...
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| Publicat a: | Brazilian Journal of Physics |
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| Autors principals: | , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Sociedade Brasileira de Física
2008
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=46413554007 |
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