Now showing items 1-4 of 4

    • Moya Fuentes, Pablo; Navarro, Roberto E. (Frontiers Media, 2021)
      Turbulence in space plasmas usually exhibits two regimes separated by a spectral break that divides the so called inertial and kinetic ranges. Large scale magnetic fluctuations are dominated by non-linear MHD wave-wave ...
    • Navarro, Roberto E.; Muñoz Gálvez, Víctor; Valdivia Hepp, Juan; Moya Fuentes, Pablo (IOP Publishing, 2020)
      Wave-particle interactions are believed to be one of the most important kinetic processes regulating the heating and acceleration of solar wind plasma. One possible explanation for the observed preferential heating of alpha ...
    • Navarro, Roberto E.; Muñoz, Víctor; Araneda, Jaime A.; Viñas, Adolfo F.; Moya, Pablo S.; Valdivia Hepp, Juan (Blackwell Publishing Ltd, 2015)
      ©2015. American Geophysical Union. All Rights Reserved. Remote and in situ observations in the solar wind show that ion and electron velocity distributions persistently present deviations from thermal equilibrium. Ion ...
    • López, Rodrigo A.; Moya Fuentes, Pablo; Navarro, Roberto; Araneda, Jaime; Muñoz Gálvez, Víctor; Viñas, Adolfo; Valdivia Hepp, Juan (IOP, 2016)
      A sufficiently large temperature anisotropy can sometimes drive various types of electromagnetic plasma micro-instabilities, which can play an important role in the dynamics of relativistic pair plasmas in space, astrophysics, ...