Se realiza una simulación de la aceleración mediante un campo eléctrico uniforme y constante (aceleración DC) que experimentarían electrones y protones al interior de una lámina de corriente durante una fulguración solar, ...

Abstract. Large amounts of energy are released when magnetic field lines reconnect in the corona during solar flares. Observations have found both transient and irreversible changes in the photospheric magnetic fields ...

During the impulsive phase of solar flares a distribution of nonthermal electrons propagates from the site of energy release towards the lower layers of the solar atmosphere. Depending on their pitch angles, these electrons ...

En el presente trabajo se abordó el problema de la variación del campo magnético y su asociación a fuentes helio-sísmicas inducidas durante fulguraciones solares mediante el estudio de uno de los mecanismos actualmente ...

This work explored the possibility of the generation of seismic signals on the Sun from a confinement of energy located in the solar interior. This idea was developed through two sections. In the first section, corresponding ...