activity
20182026
most citedSmall-scale solar jet formation and their associated waves and instabilities

16 citations · 26 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2026

Resistive MHD Simulations of Stellar Wind-Magnetosphere Coupling in TRAPPIST-1e

J. J. González-Avilés, N. Baltazar Pérez-Negrón, A. Segura

Close-in terrestrial exoplanets around M dwarfs reside in dense, magnetized winds, where non-ideal plasma coupling can strongly affect how electromagnetic energy is redistributed w…

astro-ph.SR2024★ 2 cited

Using sunRunner3D to interpret the global structure of the heliosphere from in situ measurements

José Juan González-Avilés, Pete Riley, Michal Ben-Nun +2

Understanding the large-scale three-dimensional structure of the inner heliosphere, while important in its own right, is crucial for space weather applications, such as forecasting…

astro-ph.SR2024★ 4 cited

Numerical MHD simulations of solar flares and their associated small-scale structures

Mauricio González-Servín, J. J. González-Avilés

Using numerical simulations, we study the formation and dynamics of post-flare loops in a local region of the solar atmosphere. The MHD equations rule the post-flare structures' dy…

astro-ph.SR2022★ 4 cited

Numerical simulations of a two-fluid jet at a magnetic null point in a solar arcade

J. J. González-Avilés, K. Murawski, T. V. Zaqarashvili

We study the formation and evolution of jets in the solar atmosphere using numerical simulations of partially ionized plasma. The two-fluid magnetohydrodynamic equations with ion+e…

astro-ph.SR2022★ 16 cited

Small-scale solar jet formation and their associated waves and instabilities

Samuel Skirvin, Gary Verth, José Juan González-Avilés +7

Studies on small-scale jets' formation, propagation, evolution, and role, such as type I and II spicules, mottles, and fibrils in the lower solar atmosphere's energetic balance, ha…

astro-ph.SR2018

Flows and magnetic field structures in reconnection regions of simulations of the solar atmosphere: do flux pile-up models work?

S. Shelyag, Y. E. Litvinenko, V. Fedun +3

We study the process of magnetic field annihilation and reconnection in simulations of magnetised solar photosphere and chromosphere with magnetic fields of opposite polarities and…