38 citations · 277 across the 22 of their papers we have counts for
8 papers · 1 filter
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…
H, He-like recombination spectra IV; H, He-like recombination spectra IV: clarification and refinement of methodology for -changing collisions
N. R. Badnell, F. Guzmán, S. Brodie +4
Precise spectral diagnostic modelling of H~{\sc i} and He~{\sc ii} recombination spectra can constrain theoretical models which describe many astrophysical environments. Simple ana…
Spicule jets in the solar atmosphere modeled with resistive MHD and thermal conduction
J. J. González-Avilés, F. S. Guzmán, V. Fedun +1
Using numerical simulations, we study the effects of magnetic resistivity and thermal conductivity in the dynamics and properties of solar jets with characteristics of Type II spic…
Current and future development of the photoionization code Cloudy
P. A. M. van Hoof, G. C. Van de Steene, F. Guzmán +3
The gas that is present in the interstellar medium is usually very far removed from (local) thermodynamic equilibrium, and in some cases may also not be in a steady-state equilibri…
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…
I. Jet Formation and Evolution due to 3D Magnetic Reconnection
J. J. González-Avilés, F. S. Guzmán, V. Fedun +3
Using simulated data-driven three-dimensional resistive MHD simulations of the solar atmosphere, we show that magnetic reconnection can be responsible of the formation of jets with…
Jet formation in solar atmosphere due to magnetic reconnection
J. J. González-Avilés, F. S. Guzmán, V. Fedun
Using numerical simulations, we show that jets with features of type II spicules and cold coronal jets corresponding to temperatures K can be formed due to magnetic reconn…
Newtonian CAFE: a new ideal MHD code to study the solar atmosphere
J. J. Gonzalez-Aviles, A. Cruz-Osorio, F. D. Lora-Clavijo +1
We present a new code designed to solve the equations of classical ideal magneto-hydrodynamics (MHD) in three dimensions, submitted to a constant gravitational field. The purpose o…