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CHROMOSPHERE TO 1 au SIMULATION OF THE 2011 MARCH 7th EVENT: A COMPREHENSIVE STUDY OF CORONAL MASS EJECTION PROPAGATION

The Astrophysical journal, 2017-01, Vol.834 (2), p.172

2017

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Alfvén Wave Turbulence as a Coronal Heating Mechanism: Simultaneously Predicting the Heating Rate and the Wave-induced Emission Line Broadening

The Astrophysical journal, 2017-08, Vol.845 (2), p.98

2017

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Nonequilibrium Ionization Effects on Synthetic Spectra in the AWSoM Solar Corona

The Astrophysical journal. Supplement series, 2023-12, Vol.269 (2), p.37

2023

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DATA-CONSTRAINED CORONAL MASS EJECTIONS IN A GLOBAL MAGNETOHYDRODYNAMICS MODEL

The Astrophysical journal, 2017-01, Vol.834 (2), p.173

2017

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Simulating Compressive Stream Interaction Regions during Parker Solar Probe’s First Perihelion Using Stream-aligned Magnetohydrodynamics

The Astrophysical journal, 2024-02, Vol.962 (2), p.182

2024

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Numerical Modeling of Energetic Charged-particle Transport with SPECTRUM Software: General Approach and Artificial Effects due to Field Discretization

The Astrophysical journal. Supplement series, 2024-06, Vol.272 (2), p.46

2024

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Flux rope evolution in interplanetary coronal mass ejections: the 13 May 2005 event

Plasma physics and controlled fusion, 2014-06, Vol.56 (6), p.64006-11

2014

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Predictions for the First Parker Solar Probe Encounter

Astrophysical journal. Letters, 2019-02, Vol.872 (2), p.L18

2019

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A STEADY-STATE PICTURE OF SOLAR WIND ACCELERATION AND CHARGE STATE COMPOSITION DERIVED FROM A GLOBAL WAVE-DRIVEN MHD MODEL

The Astrophysical journal, 2015-06, Vol.806 (1), p.1-25

2015

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Hybrid block-AMR in cartesian and curvilinear coordinates: MHD applications

Journal of computational physics, 2007-09, Vol.226 (1), p.925-946

2007

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CORONAL JETS SIMULATED WITH THE GLOBAL ALFVÉN WAVE SOLAR MODEL

The Astrophysical journal, 2017-01, Vol.834 (2), p.123

2017

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Charge State Calculation for Global Solar Wind Modeling

The Astrophysical journal, 2022-02, Vol.926 (1), p.35

2022

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ALFVEN WAVE SOLAR MODEL (AWSoM): CORONAL HEATING

The Astrophysical journal, 2014-02, Vol.782 (2), p.1-15

2014

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Parallel, grid-adaptive approaches for relativistic hydro and magnetohydrodynamics

Journal of computational physics, 2012-02, Vol.231 (3), p.718-744

2012

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A GLOBAL WAVE-DRIVEN MAGNETOHYDRODYNAMIC SOLAR MODEL WITH A UNIFIED TREATMENT OF OPEN AND CLOSED MAGNETIC FIELD TOPOLOGIES

The Astrophysical journal, 2013-12, Vol.778 (2), p.1-20

2013

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Alfvén wave solar model (AWSoM): proton temperature anisotropy and solar wind acceleration

Monthly notices of the Royal Astronomical Society, 2015-12, Vol.454 (4), p.3697-3709

2015

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On the effect of the initial magnetic polarity and of the background wind on the evolution of CME shocks

Astronomy and astrophysics (Berlin), 2005-03, Vol.432 (1), p.331-339

2005

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Importance of Ambipolar Electric Field in Driving Ion Loss From Mars: Results From a Multifluid MHD Model With the Electron Pressure Equation Included

Journal of geophysical research. Space physics, 2019-11, Vol.124 (11), p.9040-9057

2019

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Three‐Dimensional Structure of the Corona During WHPI Campaign Rotations CR‐2219 and CR‐2223

Journal of geophysical research. Space physics, 2022-06, Vol.127 (6), p.n/a

2022

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Improving the Alfvén Wave Solar Atmosphere Model Based on Parker Solar Probe Data

The Astrophysical journal, 2022-02, Vol.925 (2), p.146

2022

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Comparison between 2.5D and 3D simulations of coronal mass ejections

Astronomy and astrophysics (Berlin), 2007-07, Vol.470 (1), p.359-365

2007

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A Data-driven, Two-temperature Solar Wind Model with Alfvén Waves

The Astrophysical journal, 2010-12, Vol.725 (1), p.1373-1383

2010

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SPECTRUM: Synthetic Spectral Calculations for Global Space Plasma Modeling

The Astrophysical journal. Supplement series, 2019-05, Vol.242 (1), p.1

2019

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On the effect of the background wind on the evolution of interplanetary shock waves

Astronomy and astrophysics (Berlin), 2005-02, Vol.430 (3), p.1099-1107

2005

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NUMERICAL SIMULATIONS OF CORONAL MASS EJECTION ON 2011 MARCH 7: ONE-TEMPERATURE AND TWO-TEMPERATURE MODEL COMPARISON

The Astrophysical journal, 2013-08, Vol.773 (1), p.1-10

2013

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CHROMOSPHERE TO 1 au SIMULATION OF THE 2011 MARCH 7th EVENT: A COMPREHENSIVE STUDY OF CORONAL MASS EJECTION PROPAGATION

Alfvén Wave Turbulence as a Coronal Heating Mechanism: Simultaneously Predicting the Heating Rate and the Wave-induced Emission Line Broadening

Nonequilibrium Ionization Effects on Synthetic Spectra in the AWSoM Solar Corona

DATA-CONSTRAINED CORONAL MASS EJECTIONS IN A GLOBAL MAGNETOHYDRODYNAMICS MODEL

Simulating Compressive Stream Interaction Regions during Parker Solar Probe’s First Perihelion Using Stream-aligned Magnetohydrodynamics

Numerical Modeling of Energetic Charged-particle Transport with SPECTRUM Software: General Approach and Artificial Effects due to Field Discretization

Flux rope evolution in interplanetary coronal mass ejections: the 13 May 2005 event

Predictions for the First Parker Solar Probe Encounter

A STEADY-STATE PICTURE OF SOLAR WIND ACCELERATION AND CHARGE STATE COMPOSITION DERIVED FROM A GLOBAL WAVE-DRIVEN MHD MODEL

Hybrid block-AMR in cartesian and curvilinear coordinates: MHD applications

CORONAL JETS SIMULATED WITH THE GLOBAL ALFVÉN WAVE SOLAR MODEL

Charge State Calculation for Global Solar Wind Modeling

ALFVEN WAVE SOLAR MODEL (AWSoM): CORONAL HEATING

Parallel, grid-adaptive approaches for relativistic hydro and magnetohydrodynamics

A GLOBAL WAVE-DRIVEN MAGNETOHYDRODYNAMIC SOLAR MODEL WITH A UNIFIED TREATMENT OF OPEN AND CLOSED MAGNETIC FIELD TOPOLOGIES

Alfvén wave solar model (AWSoM): proton temperature anisotropy and solar wind acceleration

On the effect of the initial magnetic polarity and of the background wind on the evolution of CME shocks

Importance of Ambipolar Electric Field in Driving Ion Loss From Mars: Results From a Multifluid MHD Model With the Electron Pressure Equation Included

Three‐Dimensional Structure of the Corona During WHPI Campaign Rotations CR‐2219 and CR‐2223

Improving the Alfvén Wave Solar Atmosphere Model Based on Parker Solar Probe Data

Comparison between 2.5D and 3D simulations of coronal mass ejections

A Data-driven, Two-temperature Solar Wind Model with Alfvén Waves

SPECTRUM: Synthetic Spectral Calculations for Global Space Plasma Modeling

On the effect of the background wind on the evolution of interplanetary shock waves

NUMERICAL SIMULATIONS OF CORONAL MASS EJECTION ON 2011 MARCH 7: ONE-TEMPERATURE AND TWO-TEMPERATURE MODEL COMPARISON

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