In situ properties of small and large flux ropes in the solar wind

Two populations of twisted magnetic field tubes, or flux ropes (hereafter, FRs), are detected by in situ measurements in the solar wind. While small FRs are crossed by the observing spacecraft within few hours, with a radius typically less than 0.1 AU, larger FRs, or magnetic clouds (hereafter, MCs)...

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Detalles Bibliográficos
Autor principal:	Dasso, Sergio Ricardo
Publicado:	2014
Materias:	Flux ropes Interplanetary Coronal Mass Ejections Magnetic clouds Solar Wind
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_21699380_v119_n9_p7088_Janvier http://hdl.handle.net/20.500.12110/paper_21699380_v119_n9_p7088_Janvier
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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