In order to explain the evolution with energy of the charge state of solar par-ticles we have developed a model where charge states are defined at the source during the particle acceleration process. Charge-interchange processes between the accelerated ions and local matter are considered on basis of electron loss and capture cross-sections at high energies. The model is worked out under two different approaches. We apply the model to observational data of charge states of most of particle events published in the literature. We discuss our results and implications within the frame of other existing models: we conclude that our analyticaldeveloped by other authors
Observed charge states of solar energetic ions by Solar, Anomalous, and Magnetospheric Particle Expl...
In a nonequilibrium model that includes shock-induced acceleration, we simulate the charge state and...
We report an attempt to measure the ionic charge state of solar energetic oxygen ions at energies of...
Con objeto de reproducir la evolución con energía de los estados de carga observacionales de los ion...
Ionic charge states of solar energetic particles (SEPs) provide information about their source envir...
Ionic charge states of solar energetic particles (SEPs) provide information about their source envir...
In some large solar energetic particle (SEP) events, the intensities of higher energy SEPs decay mor...
A novel technique to infer average ionic charge states of high energy (≥ 10 MeV/nuc) solar energetic...
Direct ionic charge state measurements have been made for solar energetic particle (SEP) events by t...
We examine the range of possible energy dependence of the ionization states of ions that are shock-a...
The conditions for establishment of charge transfer during acceleration of nuclei up to Fe, for typi...
In some large solar energetic particle (SEP) events, the intensities of higher energy SEPs decay mor...
We consider a uniÐed model of Fe ion acceleration in the solar corona. The model comprises charge-ch...
The ionic charge states of solar energetic particles (SEPs) probe source-material temperatures and a...
Abstract. Ionic charge state distributions for a variety of species, such as C, O, Ne, Mg, Si and Fe...
Observed charge states of solar energetic ions by Solar, Anomalous, and Magnetospheric Particle Expl...
In a nonequilibrium model that includes shock-induced acceleration, we simulate the charge state and...
We report an attempt to measure the ionic charge state of solar energetic oxygen ions at energies of...
Con objeto de reproducir la evolución con energía de los estados de carga observacionales de los ion...
Ionic charge states of solar energetic particles (SEPs) provide information about their source envir...
Ionic charge states of solar energetic particles (SEPs) provide information about their source envir...
In some large solar energetic particle (SEP) events, the intensities of higher energy SEPs decay mor...
A novel technique to infer average ionic charge states of high energy (≥ 10 MeV/nuc) solar energetic...
Direct ionic charge state measurements have been made for solar energetic particle (SEP) events by t...
We examine the range of possible energy dependence of the ionization states of ions that are shock-a...
The conditions for establishment of charge transfer during acceleration of nuclei up to Fe, for typi...
In some large solar energetic particle (SEP) events, the intensities of higher energy SEPs decay mor...
We consider a uniÐed model of Fe ion acceleration in the solar corona. The model comprises charge-ch...
The ionic charge states of solar energetic particles (SEPs) probe source-material temperatures and a...
Abstract. Ionic charge state distributions for a variety of species, such as C, O, Ne, Mg, Si and Fe...
Observed charge states of solar energetic ions by Solar, Anomalous, and Magnetospheric Particle Expl...
In a nonequilibrium model that includes shock-induced acceleration, we simulate the charge state and...
We report an attempt to measure the ionic charge state of solar energetic oxygen ions at energies of...