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Sharp Alfvénic Impulses in the Near-Sun Solar Wind

The Astrophysical journal. Supplement series, 2020-02, Vol.246 (2), p.45

2020

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Magnetic Connectivity of the Ecliptic Plane within 0.5 au: Potential Field Source Surface Modeling of the First Parker Solar Probe Encounter

The Astrophysical journal. Supplement series, 2020-02, Vol.246 (2), p.23

2020

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The Statistical Properties of Solar Wind Temperature Parameters Near 1 au

The Astrophysical journal. Supplement series, 2018-06, Vol.236 (2), p.41

2018

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Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar Probe

The Astrophysical journal. Supplement series, 2020-02, Vol.246 (2), p.57

2020

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Observations and Modeling of Unstable Proton and α Particle Velocity Distributions in Sub-Alfvénic Solar Wind at Parker Solar Probe Perihelia

The Astrophysical journal, 2023-09, Vol.954 (2), p.109

2023

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The Effects of Nonequilibrium Velocity Distributions on Alfvén Ion-cyclotron Waves in the Solar Wind

The Astrophysical journal, 2023-10, Vol.955 (2), p.97

2023

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Ion‐driven instabilities in the solar wind: Wind observations of 19 March 2005

Journal of geophysical research. Space physics, 2016-01, Vol.121 (1), p.30-41

2016

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Helium Abundance Periods Observed by the Solar Probe Cup on Parker Solar Probe: Encounters 1–14

The Astrophysical journal, 2024-03, Vol.964 (1), p.81

2024

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Direct In Situ Measurements of a Fast Coronal Mass Ejection and Associated Structures in the Corona

The Astrophysical journal, 2024-03, Vol.963 (2), p.85

2024

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On the Evolution of the Anisotropic Scaling of Magnetohydrodynamic Turbulence in the Inner Heliosphere

The Astrophysical journal, 2023-07, Vol.951 (2), p.141

2023

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Erratum: “The Statistical Properties of Solar Wind Temperature Parameters Near 1 au” (2018, ApJS, 236, 41)

The Astrophysical journal. Supplement series, 2023-12, Vol.269 (2), p.62

2023

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Magnetic Field Spectral Evolution in the Inner Heliosphere

Astrophysical journal. Letters, 2023-01, Vol.943 (1), p.L8

2023

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The Solar Wind Angular Momentum Flux as Observed by Parker Solar Probe

Astrophysical journal. Letters, 2020-10, Vol.902 (1), p.L4

2020

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Solar Wind Helium Abundance as a Function of Speed and Heliographic Latitude: Variation through a Solar Cycle

The Astrophysical journal, 2007-05, Vol.660 (1), p.901-910

2007

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A Comparison of Alpha Particle and Proton Beam Differential Flows in Collisionally Young Solar Wind

The Astrophysical journal, 2018-09, Vol.864 (2), p.112

2018

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Spectra of Temperature Fluctuations in the Solar Wind

Atmosphere, 2021-10, Vol.12 (10), p.1277

2021

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Statistical Analysis of the Radial Evolution of the Solar Winds between 0.1 and 1 au and Their Semiempirical Isopoly Fluid Modeling

The Astrophysical journal, 2022-12, Vol.940 (2), p.130

2022

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Determination of Solar Wind Angular Momentum and Alfvén Radius from Parker Solar Probe Observations

Astrophysical journal. Letters, 2021-02, Vol.908 (2), p.L41

2021

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The Solar Probe Cup on the Parker Solar Probe

The Astrophysical journal. Supplement series, 2020-02, Vol.246 (2), p.43

2020

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Characteristic Scales of Magnetic Switchback Patches Near the Sun and Their Possible Association With Solar Supergranulation and Granulation

The Astrophysical journal, 2021-10, Vol.919 (2), p.96

2021

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Sensitive test for ion-cyclotron resonant heating in the solar wind

Physical review letters, 2013-03, Vol.110 (9), p.091102-091102, Article 091102

2013

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The Role of Alfvén Wave Dynamics on the Large-scale Properties of the Solar Wind: Comparing an MHD Simulation with Parker Solar Probe E1 Data

The Astrophysical journal. Supplement series, 2020-02, Vol.246 (2), p.24

2020

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Predicting the Magnetic Fields of a Stealth CME Detected by Parker Solar Probe at 0.5 au

The Astrophysical journal, 2021-10, Vol.920 (2), p.65

2021

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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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Sharp Alfvénic Impulses in the Near-Sun Solar Wind

Magnetic Connectivity of the Ecliptic Plane within 0.5 au: Potential Field Source Surface Modeling of the First Parker Solar Probe Encounter

The Statistical Properties of Solar Wind Temperature Parameters Near 1 au

Density Fluctuations in the Solar Wind Based on Type III Radio Bursts Observed by Parker Solar Probe

Observations and Modeling of Unstable Proton and α Particle Velocity Distributions in Sub-Alfvénic Solar Wind at Parker Solar Probe Perihelia

The Effects of Nonequilibrium Velocity Distributions on Alfvén Ion-cyclotron Waves in the Solar Wind

Ion‐driven instabilities in the solar wind: Wind observations of 19 March 2005

Helium Abundance Periods Observed by the Solar Probe Cup on Parker Solar Probe: Encounters 1–14

Direct In Situ Measurements of a Fast Coronal Mass Ejection and Associated Structures in the Corona

On the Evolution of the Anisotropic Scaling of Magnetohydrodynamic Turbulence in the Inner Heliosphere

Erratum: “The Statistical Properties of Solar Wind Temperature Parameters Near 1 au” (2018, ApJS, 236, 41)

On the Mesoscale Structure of Coronal Mass Ejections at Mercury’s Orbit: BepiColombo and Parker Solar Probe Observations

Magnetic Field Spectral Evolution in the Inner Heliosphere

The Solar Wind Angular Momentum Flux as Observed by Parker Solar Probe

Solar Wind Helium Abundance as a Function of Speed and Heliographic Latitude: Variation through a Solar Cycle

A Comparison of Alpha Particle and Proton Beam Differential Flows in Collisionally Young Solar Wind

Spectra of Temperature Fluctuations in the Solar Wind

Statistical Analysis of the Radial Evolution of the Solar Winds between 0.1 and 1 au and Their Semiempirical Isopoly Fluid Modeling

Determination of Solar Wind Angular Momentum and Alfvén Radius from Parker Solar Probe Observations

The Solar Probe Cup on the Parker Solar Probe

Characteristic Scales of Magnetic Switchback Patches Near the Sun and Their Possible Association With Solar Supergranulation and Granulation

Sensitive test for ion-cyclotron resonant heating in the solar wind

The Role of Alfvén Wave Dynamics on the Large-scale Properties of the Solar Wind: Comparing an MHD Simulation with Parker Solar Probe E1 Data

Predicting the Magnetic Fields of a Stealth CME Detected by Parker Solar Probe at 0.5 au

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

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