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THE IMPORTANCE OF GEOMETRIC EFFECTS IN CORONAL LOOP MODELS

The Astrophysical journal, 2013-08, Vol.773 (2), p.1-16

2013

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CLOSED-FIELD CORONAL HEATING DRIVEN BY WAVE TURBULENCE

The Astrophysical journal, 2016-12, Vol.832 (2), p.180

2016

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SLOW RISE AND PARTIAL ERUPTION OF A DOUBLE-DECKER FILAMENT. I. OBSERVATIONS AND INTERPRETATION

The Astrophysical journal, 2012-09, Vol.756 (1), p.1-14

2012

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Deflection of Coronal Mass Ejections in Unipolar Ambient Magnetic Fields

The Astrophysical journal, 2023-11, Vol.957 (2), p.74

2023

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Global MHD Simulations of the Time-dependent Corona

The Astrophysical journal, 2023-12, Vol.959 (2), p.77

2023

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3D MHD Time-dependent Charge State Ionization and Recombination Modeling of the Bastille Day Coronal Mass Ejection

The Astrophysical journal, 2023-09, Vol.955 (1), p.65

2023

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INFERRING THE STRUCTURE OF THE SOLAR CORONA AND INNER HELIOSPHERE DURING THE MAUNDER MINIMUM USING GLOBAL THERMODYNAMIC MAGNETOHYDRODYNAMIC SIMULATIONS

The Astrophysical journal, 2015-04, Vol.802 (2), p.1-14

2015

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Proton and Electron Temperatures in the Solar Wind and Their Correlations with the Solar Wind Speed

The Astrophysical journal, 2023-02, Vol.944 (1), p.82

2023

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Time-dependent Dynamics of the Corona

Astrophysical journal. Letters, 2023-12, Vol.959 (1), p.L4

2023

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AN INVESTIGATION OF TIME LAG MAPS USING THREE-DIMENSIONAL SIMULATIONS OF HIGHLY STRATIFIED HEATING

The Astrophysical journal, 2016-11, Vol.831 (2), p.172

2016

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THERMAL NON-EQUILIBRIUM REVISITED: A HEATING MODEL FOR CORONAL LOOPS

The Astrophysical journal, 2013-08, Vol.773 (2), p.1-10

2013

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Multispectral Emission of the Sun During the First Whole Sun Month: Magnetohydrodynamic Simulations

The Astrophysical journal, 2009-01, Vol.690 (1), p.902-912

2009

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The Formation of Coronal Loops by Thermal Instability in Three Dimensions

The Astrophysical journal, 2008-06, Vol.679 (2), p.L161-L165

2008

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Using Global Simulations to Relate the Three-Part Structure of Coronal Mass Ejections to In Situ Signatures

The Astrophysical journal, 2008-01, Vol.672 (2), p.1221-1227

2008

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Predicting the Structure of the Solar Corona and Inner Heliosphere during Parker Solar Probe's First Perihelion Pass

Astrophysical journal. Letters, 2019-04, Vol.874 (2), p.L15

2019

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VALIDATING A TIME-DEPENDENT TURBULENCE-DRIVEN MODEL OF THE SOLAR WIND

The Astrophysical journal, 2014-04, Vol.784 (2), p.1-7

2014

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Comparing and Contrasting the Properties of the Inner Heliosphere for the Three Most Recent Solar Minima

Journal of geophysical research. Space physics, 2022-08, Vol.127 (8), p.e2022JA030261-n/a

2022

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Identifying Observables That Can Differentiate Between Impulsive and Footpoint Heating: Time Lags and Intensity Ratios

The Astrophysical journal, 2018-10, Vol.865 (2), p.111

2018

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A THREE-DIMENSIONAL MODEL OF ACTIVE REGION 7986: COMPARISON OF SIMULATIONS WITH OBSERVATIONS

The Astrophysical journal, 2016-01, Vol.817 (1), p.15

2016

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Using Parker Solar Probe observations during the first four perihelia to constrain global magnetohydrodynamic models

Astronomy and astrophysics (Berlin), 2021-06, Vol.650, p.A19

2021

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APPLICATION OF A SOLAR WIND MODEL DRIVEN BY TURBULENCE DISSIPATION TO A 2D MAGNETIC FIELD CONFIGURATION

The Astrophysical journal, 2014-12, Vol.796 (2), p.1-7

2014

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Magnetic Topology of Coronal Hole Linkages

The Astrophysical journal, 2011-04, Vol.731 (2), p.111-jQuery1323909340348='48'

2011

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Fine Structures of the Inner Solar Corona and the Associated Magnetic Topology

The Astrophysical journal, 2022-07, Vol.933 (1), p.95

2022

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Constraining the CME Core Heating and Energy Budget with SOHO/UVCS

The Astrophysical journal, 2022-03, Vol.927 (1), p.27

2022

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Energetic Proton Propagation and Acceleration Simulated for the Bastille Day Event of 2000 July 14

The Astrophysical journal, 2021-03, Vol.909 (2), p.160

2021

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THE IMPORTANCE OF GEOMETRIC EFFECTS IN CORONAL LOOP MODELS

CLOSED-FIELD CORONAL HEATING DRIVEN BY WAVE TURBULENCE

SLOW RISE AND PARTIAL ERUPTION OF A DOUBLE-DECKER FILAMENT. I. OBSERVATIONS AND INTERPRETATION

Deflection of Coronal Mass Ejections in Unipolar Ambient Magnetic Fields

Global MHD Simulations of the Time-dependent Corona

3D MHD Time-dependent Charge State Ionization and Recombination Modeling of the Bastille Day Coronal Mass Ejection

INFERRING THE STRUCTURE OF THE SOLAR CORONA AND INNER HELIOSPHERE DURING THE MAUNDER MINIMUM USING GLOBAL THERMODYNAMIC MAGNETOHYDRODYNAMIC SIMULATIONS

Proton and Electron Temperatures in the Solar Wind and Their Correlations with the Solar Wind Speed

Time-dependent Dynamics of the Corona

AN INVESTIGATION OF TIME LAG MAPS USING THREE-DIMENSIONAL SIMULATIONS OF HIGHLY STRATIFIED HEATING

THERMAL NON-EQUILIBRIUM REVISITED: A HEATING MODEL FOR CORONAL LOOPS

Multispectral Emission of the Sun During the First Whole Sun Month: Magnetohydrodynamic Simulations

The Formation of Coronal Loops by Thermal Instability in Three Dimensions

Using Global Simulations to Relate the Three-Part Structure of Coronal Mass Ejections to In Situ Signatures

Predicting the Structure of the Solar Corona and Inner Heliosphere during Parker Solar Probe's First Perihelion Pass

VALIDATING A TIME-DEPENDENT TURBULENCE-DRIVEN MODEL OF THE SOLAR WIND

Comparing and Contrasting the Properties of the Inner Heliosphere for the Three Most Recent Solar Minima

Identifying Observables That Can Differentiate Between Impulsive and Footpoint Heating: Time Lags and Intensity Ratios

A THREE-DIMENSIONAL MODEL OF ACTIVE REGION 7986: COMPARISON OF SIMULATIONS WITH OBSERVATIONS

Using Parker Solar Probe observations during the first four perihelia to constrain global magnetohydrodynamic models

APPLICATION OF A SOLAR WIND MODEL DRIVEN BY TURBULENCE DISSIPATION TO A 2D MAGNETIC FIELD CONFIGURATION

Magnetic Topology of Coronal Hole Linkages

Fine Structures of the Inner Solar Corona and the Associated Magnetic Topology

Constraining the CME Core Heating and Energy Budget with SOHO/UVCS

Energetic Proton Propagation and Acceleration Simulated for the Bastille Day Event of 2000 July 14

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