Progressive transformation of a flux rope to an ICME : CCComparative analysis using the direct and fitted expansion methods

Mostrar todas las versiones(2)

The solar wind conditions at one astronomical unit (AU) can be strongly disturbed by interplanetary coronal mass ejections (ICMEs). A subset, called magnetic clouds (MCs), is formed by twisted flux ropes that transport an important amount of magnetic flux and helicity, which is released in CMEs. At...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Dasso, S., Nakwacki, M.S., Démoulin, P., Mandrini, C.H.
Formato: JOUR
Materias:
Coronal mass ejection: interplanetary
Magnetic fields: interplanetary
Magnetic reconnection: observational signatures
Solar wind: disturbances
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00380938_v244_n1-2_p115_Dasso
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

Ejemplares similares

Ejemplares similares