Browsing by Author "Moya Fuentes, Pablo Sebastián"
Now showing items 1-7 of 7
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López, Rodrigo A.; Moya Fuentes, Pablo Sebastián; Shaaban, Shaaban M.; Lazar, Marian; Yoon, Peter H.; Poedts, Stefaan (Springer, 2021)In this chapter we focus on the recent progress made on numerical analysis and tools facilitating the investigation of dispersion and stability of anisotropic Kappa distributed plasmas. Plasma waves and fluctuations are ...
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Assigning degrees of stochasticity to blazar light curves in the radio band using complex networks Acosta Tripailao, Belén; Max-Moerbeck Astudillo, Walter Kennerth; Pastén Guzmán, Denisse Elizabeth del Carmen; Moya Fuentes, Pablo Sebastián (MDPI, 2022)We focus on characterizing the high-energy emission mechanisms of blazars by analyzing the variability in the radio band of the light curves of more than a thousand sources. We are interested in assigning complexity ...
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Silva Navarrete, Javier Ignacio (Universidad de Chile, 2023)Utilizando datos de la misión espacial Wind, llevamos a cabo un estudio de los procesos de transporte de energía mediado por electrones del viento solar. La investigación se dividió en dos enfoques: uno macroscópico y ...
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Reyes, Paula I.; Pinto, Víctor A.; Moya Fuentes, Pablo Sebastián (Amer Geophysical Union, 2021)Using a time series of geomagnetic storm events between 1957 and 2019, obtained by selecting storms where Dst<-50 nT, we have analyzed the probability of occurrence of moderate, intense, and severe events. Considering that ...
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Gallo Méndez, Iván Andrés (Universidad de Chile, 2024)Turbulence, a ubiquitous and intricate phenomenon that manifests across diverse systems, has been studied using many tools with robust frameworks for understanding complex dynamics with high degrees of freedom. Within this ...
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Zenteno Quinteros, Beatriz Antonia; Viñas, Adolfo; Moya Fuentes, Pablo Sebastián (IOP Publishing, 2021)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 and strahl. Skewness may provide energy for ...
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Zenteno Quinteros, Beatriz Antonia; Moya Fuentes, Pablo Sebastián (Frontiers Media, 2022)There is wide observational evidence that electron velocity distribution functions (eVDF) observed in the solar wind generally present enhanced tails and field-aligned skewness. These properties may induce the excitation ...