Typical Profiles and Distributions of Plasma and Magnetic Field Parameters in Magnetic Clouds at 1 AU

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Magnetic clouds (MCs) are a subset of interplanetary coronal mass ejections (ICMEs). They are important because of their simple internal magnetic field configuration, which resembles a magnetic flux rope, and because they represent one of the most geoeffective types of solar transients. In this stud...

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Detalles Bibliográficos
Autores principales: Rodriguez, L., Masías-Meza, J.J., Dasso, S., Démoulin, P., Zhukov, A.N., Gulisano, A.M., Mierla, M., Kilpua, E., West, M., Lacatus, D., Paraschiv, A., Janvier, M.
Formato: JOUR
Materias:
Coronal mass ejections, low coronal signatures, initiation and propagation
Interplanetary coronal mass ejections
Magnetic clouds
Space weather
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00380938_v291_n7_p2145_Rodriguez
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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