Disipación de Turbulencia en Plasmas Astrofísicos, Conexión entre Fluctuaciones Microscópicas y MacroscópicasRoberto E. Navarro2018 - 2020PAI No. 79170095, ANID-ChileAssociated publicationsPablo S. Moya, Roberto E. Navarro (2021). Effects of the Background Turbulence on the Relaxation of Ion Temperature Anisotropy in Space Plasmas. Front. Phys. 9, 175.PDF Cite DOIRoberto E. Navarro, Víctor Muñoz, Juan A Valdivia, Pablo S Moya (2020). Feasibility of Ion-cyclotron Resonant Heating in the Solar Wind. Astrophys. J. 898, L9.PDF Cite DOIRoberto E. NavarroAssistant ProfessorPhD in Sciences w/m Physics | Professor at UdeC | Research on Plasma Physics | Linux User & dog lover | Haven’t watched any Star Wars movieNextKinetic instabilities and wave-particle interactions in non Maxwellian plasmas. Linear, quasi-linear, and non-linear analysisPreviousTurbulence Dissipation Between Macroscopic and Kinetic Scales in Astrophysical Plasmas