Why are CMEs large-scale coronal events: Nature or nurture?
The apparent contradiction between small-scale source regions of, and large-scale coronal response to, coronal mass ejections (CMEs) has been a long-standing puzzle. For some, CMEs are considered to be inherently large-scale events ĝ€" eruptions in which a number of flux systems participate in...
Guardado en:
Autores principales: | Van Driel-Gesztelyi, L., Attrill, G.D.R., Démoulin, P., Mandrini, C.H., Harra, L.K. |
---|---|
Formato: | JOUR |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_09927689_v26_n10_p3077_VanDrielGesztelyi |
Aporte de: |
Ejemplares similares
-
Why are CMEs large-scale coronal events: Nature or nurture?
Publicado: (2008) -
The long-term evolution of AR 7978: The scalings of the coronal plasma parameters with the mean photospheric magnetic field
por: Van Driel-Gesztelyi, L., et al. -
Oxygen abundance variations in coronal streamers affected by CMES
Publicado: (2006) -
Oxygen abundance variations in coronal streamers affected by CMES
por: Vásquez, A.M., et al. -
Magnetic field and plasma scaling laws: Their implications for coronal heating models
por: Mandrini, C.H., et al.