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Numerical MHD models of stream interaction regions (SIRs) and corotating interaction regions (CIRs) using sunRunner3D: comparison with observations

Monthly notices of the Royal Astronomical Society, 2024-03, Vol.529 (2), p.1250-1257

2024

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Numerical simulations of macrospicule jets under energy imbalance conditions in the solar atmosphere

Monthly notices of the Royal Astronomical Society, 2021-07, Vol.505 (1), p.50-64

2021

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I. Jet Formation and Evolution Due to 3D Magnetic Reconnection

The Astrophysical journal, 2018-04, Vol.856 (2), p.176

2018

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In situ generation of coronal Alfvén waves by jets

Monthly notices of the Royal Astronomical Society, 2019-04, Vol.484 (2), p.1936-1945

2019

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

Astronomy and astrophysics (Berlin), 2018-12, Vol.620, p.A159

2018

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Stability of BEC galactic dark matter halos

Journal of cosmology and astroparticle physics, 2013-09, Vol.2013 (9), p.34-34

2013

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Historical differences in temperature between urban and non‐urban areas in Puerto Rico

International journal of climatology, 2015-06, Vol.35 (7), p.1648-1661

2015

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Modos de ondas magnetohidrodinámicas influenciados por la corriente de desplazamiento

Revista Brasileira de Ensino de Física, 2021, Vol.43

2021

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Propagation of Type II spicules into the solar corona I. A Thermomechanical toy model (Plasma rise phase)

Journal of physics. Conference series, 2022-09, Vol.2307 (1), p.12063

2022

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Propagation of Type II spicules into the solar corona III. MHD simulation

Journal of physics. Conference series, 2022-09, Vol.2307 (1), p.12065

2022

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Propagation of Type II spicules into the solar corona II. A Thermomechanical toy model (Plasma escape and descent phase)

Journal of physics. Conference series, 2022-09, Vol.2307 (1), p.12064

2022

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Spectroscopic Study of Solar Transition Region Oscillations in the Quiet-Sun Observed By IRIS Using Si IV Spectral Line

Monthly notices of the Royal Astronomical Society, 2022-10, Vol.517 (1), p.458-473

2022

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Expériences langagières réflexives dans un monde nahua divers : De la stigmatisation sociolinguistique à la dialectologie sociale appliquée

Signifiances (Signifying), 2022-06, Vol.5 (1), p.67-83

Avilés González, Karla J.

2022

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

Monthly notices of the Royal Astronomical Society, 2024-02, Vol.528 (3), p.5098-5113

2024

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JET Formation in Solar Atmosphere Due to Magnetic Reconnection

The Astrophysical journal, 2017-02, Vol.836 (1), p.24

2017

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

Monthly notices of the Royal Astronomical Society, 2022-08, Vol.515 (4), p.5094-5105

2022

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A Semi-empirical Approach to the Dynamic Coupling of CMEs and Solar Wind

The Astrophysical journal, 2022-09, Vol.937 (1), p.24

2022

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Spicule Jets in the Solar Atmosphere Modeled with Resistive MHD and Thermal Conduction

The Astrophysical journal, 2020-07, Vol.897 (2), p.153

2020

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Numerical MHD Simulations of Reconnection in Solar Flares: Effects of the Magnetic-Field Strength in the Current Sheet

Solar physics, 2023-09, Vol.298 (9), p.109, Article 109

2023

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R. Aída Hernández Castillo, Suzi Hutchings & Brian Noble (dir.), Transcontinental Dialogues. Activist Alliances with Indigenous Peoples of Canada, Mexico, and Australia: Tucson, The University of Arizona Press, 2019

Cahiers des amériques latines (Paris), 2021-10 (96), p.226-229

Avilés González, Karla J.

2021

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Newtonian cafe: a new ideal MHD code to study the solar atmosphere

Monthly notices of the Royal Astronomical Society, 2015-12, Vol.454 (2), p.1871-1885

2015

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Estimating the contribution of Alfvén waves to the process of heating the quiet solar corona

Monthly notices of the Royal Astronomical Society, 2015-07, Vol.451 (1), p.300-311

2015

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Investigating the effects of numerical algorithms on global magnetohydrodynamics simulations of solar wind in the inner heliosphere

Revista mexicana de física, 2024-05, Vol.70 (3 May-Jun)

2024

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Thermal model of a solar concentration cooker: a parameter variation study to estimate thermal properties

Revista internacional de métodos numéricos para cálculo y diseno en ingenieria, 2019

2019

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Historical differences in temperature between urban and non-urban areas in Puerto Rico: URBAN versus NON-URBAN TEMPERATURES IN PUERTO RICO

International journal of climatology, 2015-06, Vol.35 (7), p.1648-1661

2015

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Numerical MHD models of stream interaction regions (SIRs) and corotating interaction regions (CIRs) using sunRunner3D: comparison with observations

Numerical simulations of macrospicule jets under energy imbalance conditions in the solar atmosphere

I. Jet Formation and Evolution Due to 3D Magnetic Reconnection

In situ generation of coronal Alfvén waves by jets

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

Stability of BEC galactic dark matter halos

Historical differences in temperature between urban and non‐urban areas in Puerto Rico

Modos de ondas magnetohidrodinámicas influenciados por la corriente de desplazamiento

Propagation of Type II spicules into the solar corona I. A Thermomechanical toy model (Plasma rise phase)

Propagation of Type II spicules into the solar corona III. MHD simulation

Propagation of Type II spicules into the solar corona II. A Thermomechanical toy model (Plasma escape and descent phase)

Spectroscopic Study of Solar Transition Region Oscillations in the Quiet-Sun Observed By IRIS Using Si IV Spectral Line

Expériences langagières réflexives dans un monde nahua divers : De la stigmatisation sociolinguistique à la dialectologie sociale appliquée

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

JET Formation in Solar Atmosphere Due to Magnetic Reconnection

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

A Semi-empirical Approach to the Dynamic Coupling of CMEs and Solar Wind

Spicule Jets in the Solar Atmosphere Modeled with Resistive MHD and Thermal Conduction

Numerical MHD Simulations of Reconnection in Solar Flares: Effects of the Magnetic-Field Strength in the Current Sheet

R. Aída Hernández Castillo, Suzi Hutchings & Brian Noble (dir.), Transcontinental Dialogues. Activist Alliances with Indigenous Peoples of Canada, Mexico, and Australia: Tucson, The University of Arizona Press, 2019

Newtonian cafe: a new ideal MHD code to study the solar atmosphere

Estimating the contribution of Alfvén waves to the process of heating the quiet solar corona

Investigating the effects of numerical algorithms on global magnetohydrodynamics simulations of solar wind in the inner heliosphere

Thermal model of a solar concentration cooker: a parameter variation study to estimate thermal properties

Historical differences in temperature between urban and non-urban areas in Puerto Rico: URBAN versus NON-URBAN TEMPERATURES IN PUERTO RICO

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