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Switchbacks in the Near-Sun Magnetic Field: Long Memory and Impact on the Turbulence Cascade

The Astrophysical journal. Supplement series, 2020-02, Vol.246 (2), p.39

2020

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PROPINQUITY OF CURRENT AND VORTEX STRUCTURES: EFFECTS ON COLLISIONLESS PLASMA HEATING

The Astrophysical journal, 2016-11, Vol.832 (1), p.57

2016

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Relativistic Particle Transport and Acceleration in Structured Plasma Turbulence

The Astrophysical journal, 2022-03, Vol.928 (1), p.25

2022

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The Steady Global Corona and Solar Wind: A Three-dimensional MHD Simulation with Turbulence Transport and Heating

The Astrophysical journal, 2018-09, Vol.865 (1), p.25

2018

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Pathways to Dissipation in Weakly Collisional Plasmas

The Astrophysical journal, 2020-03, Vol.891 (1), p.101

2020

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Novel perspectives on stomatal impressions: Rapid and non-invasive surface characterization of plant leaves by scanning electron microscopy

PloS one, 2020-09, Vol.15 (9), p.e0238589

2020

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Subproton-scale Intermittency in Near-Sun Solar Wind Turbulence Observed by the Parker Solar Probe

Astrophysical journal. Letters, 2021-04, Vol.911 (1), p.L7

2021

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Quantifying the Agyrotropy of Proton and Electron Heating in Turbulent Plasmas

The Astrophysical journal, 2023-02, Vol.944 (2), p.148

2023

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THREE-FLUID, THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SOLAR WIND MODEL WITH EDDY VISCOSITY AND TURBULENT RESISTIVITY

The Astrophysical journal, 2014-06, Vol.788 (1), p.1-18

2014

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Dependence of Kinetic Plasma Turbulence on Plasma β

Astrophysical journal. Letters, 2018-09, Vol.864 (1), p.L21

2018

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Contextual Predictions for Parker Solar Probe. II. Turbulence Properties and Taylor Hypothesis

The Astrophysical journal. Supplement series, 2019-05, Vol.242 (1), p.12

2019

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Intermittency in the Expanding Solar Wind: Observations from Parker Solar Probe (0.16 au), Helios 1 (0.3–1 au), and Voyager 1 (1–10 au)

The Astrophysical journal. Supplement series, 2022-03, Vol.259 (1), p.23

2022

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Scale dependence of energy transfer in turbulent plasma

Monthly notices of the Royal Astronomical Society, 2019-02, Vol.482 (4), p.4933-4940

2019

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TURBULENCE AND PROTON-ELECTRON HEATING IN KINETIC PLASMA

Astrophysical journal. Letters, 2016-08, Vol.827 (1), p.L7-L7

2016

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Large-scale Structure and Turbulence Transport in the Inner Solar Wind: Comparison of Parker Solar Probe’s First Five Orbits with a Global 3D Reynolds-averaged MHD Model

The Astrophysical journal, 2021-12, Vol.923 (1), p.89

2021

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Variation in Path Lengths of Turbulent Magnetic Field Lines and Solar Energetic Particles

The Astrophysical journal, 2024-06, Vol.967 (2), p.97

2024

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Energy budget in decaying compressible MHD turbulence

Journal of fluid mechanics, 2021-04, Vol.916, Article A4

2021

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Scale and Time Dependence of Alfvénicity in the Solar Wind as Observed by the Parker Solar Probe

The Astrophysical journal, 2024-02, Vol.962 (1), p.37

2024

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Evolution of similarity lengths in anisotropic magnetohydrodynamic turbulence

Journal of fluid mechanics, 2019-10, Vol.876, p.5-18

2019

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Pressure–Strain Interaction as the Energy Dissipation Estimate in Collisionless Plasma

The Astrophysical journal, 2022-04, Vol.929 (2), p.142

2022

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A FOUR-FLUID MHD MODEL OF THE SOLAR WIND/INTERSTELLAR MEDIUM INTERACTION WITH TURBULENCE TRANSPORT AND PICKUP PROTONS AS SEPARATE FLUID

The Astrophysical journal, 2016-03, Vol.820 (1), p.17-17

2016

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Energy transfer and third-order law in forced anisotropic magneto-hydrodynamic turbulence with hyper-viscosity

Journal of fluid mechanics, 2023-10, Vol.974, Article A20

2023

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Contextual Predictions for the Parker Solar Probe. I. Critical Surfaces and Regions

The Astrophysical journal. Supplement series, 2019-03, Vol.241 (1), p.11

2019

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An extended and fragmented Alfvén zone in the Young Solar Wind

Monthly notices of the Royal Astronomical Society, 2022-04, Vol.513 (1), p.159-167

2022

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Statistics of Kinetic Dissipation in the Earth’s Magnetosheath: MMS Observations

Physical review letters, 2020-06, Vol.124 (25), p.1-255101, Article 255101

2020

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Switchbacks in the Near-Sun Magnetic Field: Long Memory and Impact on the Turbulence Cascade

PROPINQUITY OF CURRENT AND VORTEX STRUCTURES: EFFECTS ON COLLISIONLESS PLASMA HEATING

Relativistic Particle Transport and Acceleration in Structured Plasma Turbulence

The Steady Global Corona and Solar Wind: A Three-dimensional MHD Simulation with Turbulence Transport and Heating

Pathways to Dissipation in Weakly Collisional Plasmas

Novel perspectives on stomatal impressions: Rapid and non-invasive surface characterization of plant leaves by scanning electron microscopy

Subproton-scale Intermittency in Near-Sun Solar Wind Turbulence Observed by the Parker Solar Probe

Quantifying the Agyrotropy of Proton and Electron Heating in Turbulent Plasmas

THREE-FLUID, THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SOLAR WIND MODEL WITH EDDY VISCOSITY AND TURBULENT RESISTIVITY

Dependence of Kinetic Plasma Turbulence on Plasma β

Contextual Predictions for Parker Solar Probe. II. Turbulence Properties and Taylor Hypothesis

Intermittency in the Expanding Solar Wind: Observations from Parker Solar Probe (0.16 au), Helios 1 (0.3–1 au), and Voyager 1 (1–10 au)

Scale dependence of energy transfer in turbulent plasma

TURBULENCE AND PROTON-ELECTRON HEATING IN KINETIC PLASMA

Large-scale Structure and Turbulence Transport in the Inner Solar Wind: Comparison of Parker Solar Probe’s First Five Orbits with a Global 3D Reynolds-averaged MHD Model

Variation in Path Lengths of Turbulent Magnetic Field Lines and Solar Energetic Particles

Energy budget in decaying compressible MHD turbulence

Scale and Time Dependence of Alfvénicity in the Solar Wind as Observed by the Parker Solar Probe

Evolution of similarity lengths in anisotropic magnetohydrodynamic turbulence

Pressure–Strain Interaction as the Energy Dissipation Estimate in Collisionless Plasma

A FOUR-FLUID MHD MODEL OF THE SOLAR WIND/INTERSTELLAR MEDIUM INTERACTION WITH TURBULENCE TRANSPORT AND PICKUP PROTONS AS SEPARATE FLUID

Energy transfer and third-order law in forced anisotropic magneto-hydrodynamic turbulence with hyper-viscosity

Contextual Predictions for the Parker Solar Probe. I. Critical Surfaces and Regions

An extended and fragmented Alfvén zone in the Young Solar Wind

Statistics of Kinetic Dissipation in the Earth’s Magnetosheath: MMS Observations

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