Exploring the biases of a new method based on minimum variance for interplanetary magnetic clouds

Context. Magnetic clouds (MCs) are twisted magnetic structures ejected from the Sun and probed by in situ instruments. They are typically modeled as flux ropes (FRs). Aims. Magnetic field measurements are only available along the 1D spacecraft trajectory. The determination of the FR global character...

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Guardado en:
Detalles Bibliográficos
Publicado: 2018
Materias:
Magnetic fields
Sun: coronal mass ejections (CMEs)
Sun: heliosphere
Eigenvalues and eigenfunctions
Rope
Axis orientation
In-situ instruments
Magnetic clouds
Minimum variance
Spacecraft trajectories
Sun: coronal mass ejection
Temporal profile
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v619_n_p_Demoulin
http://hdl.handle.net/20.500.12110/paper_00046361_v619_n_p_Demoulin
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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