Now showing items 1-3 of 3

    • López, R. A.; Lazar, M.; Shaaban, S. M.; Poedts, S.; Moya Fuentes, Pablo (IOP Publishing, 2020)
      Heat transport in the solar wind is dominated by suprathermal electron populations, i.e., a tenuous halo and a field-aligned beam/strahl, with high energies and antisunward drifts along the magnetic field. Their evolution ...
    • Muñoz Gálvez, Víctor; Asenjo, F. A.; Domínguez, M.; López, R. A.; Valdivia Hepp, Juan; Viñas, A.; Hada, T. (European Geosciences Union&the American Geophysical Union, 2014)
      Abstract. Propagation of large-amplitude waves in plasmas is subject to several sources of nonlinearity due to relativistic effects, either when particle quiver velocities in the wave field are large, or when thermal ...
    • Valdivia Hepp, Juan; Toledo Cabrera, Benjamín; Gallo, N.; Muñoz Gálvez, Víctor; Rogan Castillo, José; Stepanova, M.; Moya Fuentes, Pablo; Navarro, R. E.; Viñas, A. F.; Araneda, J.; López, R. A.; Díaz, M. (Elsevier, 2016)
      The observations in the solar wind, which are usually organized in a beta-anisotropy diagram, seem to be constrained by linear instability thresholds. Unexpectedly, under these quasi-stable conditions, there is a finite ...