10 citations · 10 across the 5 of their papers we have counts for
5 papers
Interplay Between Anisotropy- and Skewness-driven Whistler Instabilities in the Solar Wind under the Core-Strahlo model
Bea Zenteno-Quinteros, Pablo S Moya, Marian Lazar +2
Temperature anisotropy and field-aligned skewness are commonly observed non-thermal features in electron velocity distributions in the solar wind. These characteristics can act as…
The role of O+ and He+ on the propagation of Kinetic Alfvén Waves in the Earth's inner magnetosphere
Pablo S Moya, Bea Zenteno-Quinteros, Iván Gallo-Méndez +1
Interactions between plasma particles and electromagnetic waves play a crucial role in the dynamics and regulation of the state of space environments. From plasma physics theory, t…
The role of core and strahlo electrons properties on the whistler heat-flux instability thresholds in the solar wind
Bea Zenteno-Quinteros, Pablo S. Moya
There is wide observational evidence that electron velocity distribution functions (eVDF) observed in the solar wind generally present enhanced tails and field-aligned skewness. Th…
Skew-Kappa distribution functions & whistler-heat-flux instability in the solar wind: the core-strahlo model
Bea Zenteno-Quinteros, Adolfo F. Viñas, Pablo S. Moya
Electron velocity distributions in the solar wind are known to have field-aligned skewness, which has been characterized by the presence of secondary populations such as the halo a…
The effect of oxygen ions on the stability and polarization of Kinetic Alfvén Waves in the Magnetosphere
Pablo S. Moya, Iván Gallo-Méndez, Bea Zenteno-Quinteros
One of the most striking properties of Kinetic Alfvén Waves (KAW) is that, unlike the also Alfvénic Electromagnetic Ion Cyclotron (EMIC) waves, these waves are right-hand polarized…