Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutora: Maria dels Àngels Aran SensatThe transport of solar energetic particles (SEPs) in the interplanetary space is mainly described by the competition between two processes: adiabatic focusing and pitch-angle scattering off irregularities of the mean large-scale interplanetary magnetic field. The purpose of this work is the analysis of the particle directional intensities measured during 2011 November 3 and 2010 August 14 SEP events in order to extract information of the transport processes undergone by the particles. This work involves the use of in-situ particle and solar wind plasma measurements from the Wind spacecraft
Solar energetic particles (SEPs), accelerated during solar eruptions, propagate in turbulent solar w...
The scenario and fundamentals of the physics of charged particle interplanetary transport are briefl...
Solar energetic particle (SEP) pitch-angle distributions are shaped by the competing effects of magn...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutora:...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutora:...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2014, Tutor: B...
Pitch angle distributions of solar energetic particles (SEPs) in interplanetary space sometimes exhi...
Pitch angle distributions of solar energetic particles (SEPs) in interplanetary space sometimes exhi...
An approximate solution of the Fokker-Planck equation containing pitch angle scattering and adiabati...
We study the transport of solar energetic particles (SEPs) in the inner heliosphere in order to rela...
We study the transport of solar energetic particles (SEPs) in the inner heliosphere in order to rela...
As solar energetic particles (SEPs) travel through interplanetary space, their pitch-angle distribut...
As solar energetic particles (SEPs) travel through interplanetary space, their pitch-angle distribut...
Solar energetic particles (SEPs), accelerated during solar eruptions, propagate in turbulent solar w...
Solar energetic particle (SEP) pitch-angle distributions are shaped by the competing effects of magn...
Solar energetic particles (SEPs), accelerated during solar eruptions, propagate in turbulent solar w...
The scenario and fundamentals of the physics of charged particle interplanetary transport are briefl...
Solar energetic particle (SEP) pitch-angle distributions are shaped by the competing effects of magn...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutora:...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutora:...
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Any: 2014, Tutor: B...
Pitch angle distributions of solar energetic particles (SEPs) in interplanetary space sometimes exhi...
Pitch angle distributions of solar energetic particles (SEPs) in interplanetary space sometimes exhi...
An approximate solution of the Fokker-Planck equation containing pitch angle scattering and adiabati...
We study the transport of solar energetic particles (SEPs) in the inner heliosphere in order to rela...
We study the transport of solar energetic particles (SEPs) in the inner heliosphere in order to rela...
As solar energetic particles (SEPs) travel through interplanetary space, their pitch-angle distribut...
As solar energetic particles (SEPs) travel through interplanetary space, their pitch-angle distribut...
Solar energetic particles (SEPs), accelerated during solar eruptions, propagate in turbulent solar w...
Solar energetic particle (SEP) pitch-angle distributions are shaped by the competing effects of magn...
Solar energetic particles (SEPs), accelerated during solar eruptions, propagate in turbulent solar w...
The scenario and fundamentals of the physics of charged particle interplanetary transport are briefl...
Solar energetic particle (SEP) pitch-angle distributions are shaped by the competing effects of magn...