53 citations · 204 across the 9 of their papers we have counts for
10 papers
Bridging the gap between stars and planets
Aina Palau, Dimitris Stamatellos, Matthew Bate +58
The formation mechanisms of brown dwarfs (BDs) and free-floating planets (FFPs) are poorly constrained. The two main competing scenarios include the star-like scenario, where these…
Influence of the magnetic field topology in the evolution of small-scale two-fluid jets in the solar atmosphere
E. E. Díaz-Figueroa, G. Ares de Parga, J. J. González-Avilés
We perform a series of numerical simulations to recreate small-scale two-fluid jets using the JOANNA code, considering the magnetohydrodynamics of two fluids (ions + electrons and…
Numerical simulations of macrospicule jets under energy imbalance conditions in the solar atmosphere
J. J. González-Avilés, K. Murawski, A. K. Srivastava +2
Using numerical simulations, we study the effects of thermal conduction and radiative cooling on the formation and evolution of solar jets with some macrospicules features. We init…
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…
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…
Estimating the contribution of Alfvén waves to the process of heating the quiet solar corona
J. J. Gonzalez-Aviles, F. S. Guzman
We solve numerically the ideal MHD equations with an external gravitational field in 2D in order to study the effects of impulsively generated linear and non-linear Alfvén waves in…
Rotation curves of rotating galactic BEC dark matter halos
F. S. Guzman, F. D. Lora-Clavijo, J. J. Gonzalez-Aviles +1
We present the dynamics of rotating Bose Condensate galactic dark matter halos, made of an ultralight spinless boson. We restrict to the case of adding axisymmetric rigid rotation…
Stability of BEC galactic dark matter halos
F. S. Guzman, F. D. Lora-Clavijo, J. J. Gonzalez-Aviles +1
In this paper we show that spherically symmetric BEC dark matter halos, with the density profile, that accurately fit galactic rotation curves and represent a potential…