The interplanetary magnetic structure that guides solar relativistic particles

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Context. Relating in-situ measurements of relativistic solar particles to their parent activity in the corona requires understanding the magnetic structures that guide them from their acceleration site to the Earth. Relativistic particle events are observed at times of high solar activity, when tran...

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Autores principales: Masson, S., Démoulin, P., Dasso, S., Klein, K.-L.
Formato: Artículo publishedVersion
Publicado: 2012
Materias:
methods: data analysis
solar-terrestrial relations
Sun: heliosphere
Activity cycles
Arrival time
Energetic particle measurement
Energetic particles
Fast solar winds
High-energy particles
In-situ measurement
Interplanetary coronal mass ejections
Interplanetary magnetic fields
Methods:data analysis
Neutron monitors
Parker spiral
Path length
Pitch-angle scattering
Plasma parameter
Radio bursts
Relativistic particles
Relativistic solar particles
Solar activity
Solar-terrestrial relations
Transient structure
Velocity dispersion
Electron beams
Magnetic bubbles
Magnetic fields
Magnetic structure
Magnetoplasma
Relativity
Solar energy
Solar radiation
Solar system
Solar wind
Interplanetary spacecraft
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v538_n_p_Masson
https://repositoriouba.sisbi.uba.ar/gsdl/cgi-bin/library.cgi?a=d&c=artiaex&d=paper_00046361_v538_n_p_Masson_oai
Aporte de:
Repositorio Digital de la Universidad de Buenos Aires (UBA) de Universidad de Buenos Aires

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