David McComas

Professor

Princeton University

United States

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About

David McComas is a Professor at Princeton University in the United States. His research focuses on solar wind interactions, heliospheric dynamics, and magnetospheric physics, as evidenced by his recent articles on interstellar helium scattering, switchback origins, and energetic proton temperatures. He actively contributes to understanding the magnetic field behavior beyond the heliosphere and the characteristics of the inner zodiacal cloud.

Articles (30)

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View details

André Galli

University of Bern

SWITZERLAND

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Ratan Kumar Bera

University of Alabama in Huntsville

UNITED STATES

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Smithsonian Institution

UNITED STATES

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Riddhi Bandyopadhyay

Assistant Professor

University of Delaware

UNITED STATES

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Ali Sulaiman

University of Minnesota

UNITED STATES

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David McComas

Research Interests

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About

Articles (30)

IBEX Observations of Elastic Scattering of Interstellar Helium by Solar Wind Particles

Asymmetric Tangential Velocity inside Switchbacks: Implication for Switchback Origin

Energetic Protons in the Inner Heliosphere Exhibit Consistent ∼1 MeV Temperatures

Cold and Hot Electron Populations Observed by Juno‐JADE in the Jovian Magnetodisc

Intermittency in Voyager’s Magnetic Field Beyond the Heliosphere

Meteoroid Streams Sculpt the Inner Zodiacal Cloud

Thermodynamic Constraints on Solar Wind Radial Profiles

12 yr Full Solar Cycle Maps from IBEX-Lo Interstellar Neutral Atom Observations (2009–2020)

Energetic Neutral Atom Fluxes from the Voyager 1 and 2 Directions

Predictions for New Horizons’ SWAP Measurements Downstream of the Heliospheric Termination Shock

Observations of the 2022 September 5 Solar Energetic Particle Event at 15 Solar Radii

Resonant Plasma Acceleration at Jupiter Driven by Satellite‐Magnetosphere Interactions

Observations of Kappa Distributions in Solar Energetic Protons and Derived Thermodynamic Properties

Kappa-tail Technique: Modeling and Application to Solar Energetic Particles Observed by Parker Solar Probe

Persistent Behavior in Solar Energetic Particle Time Series

IS⊙IS Solar γ-Ray Measurements: Initial Observations and Calibrations

Thermodynamics of Pickup Ions in the Heliosphere

Correlation of Coronal Mass Ejection Shock Temperature with Solar Energetic Particle Intensity

Likely Common Coronal Source of Solar Wind and 3He-enriched Energetic Particles: Uncoupled Transport from the Low Corona to 0.2 au

Oxygen production from dissociation of Europa’s water-ice surface

The Role of Pickup Ions in the Interaction of the Solar Wind with the Local Interstellar Medium. I. Importance of Kinetic Processes at the Heliospheric Termination Shock

Transport Equation of Kappa Distributions in the Heliosphere

Variation of Hydrogen Energetic Neutral Atom Flux in the Subsolar Magnetosheath as a Function of Solar Cycle

Interstellar Conditions Deduced from Interstellar Neutral Helium Observed by IBEX and Global Heliosphere Modeling

Theory and Transport of Nearly Incompressible Magnetohydrodynamic Turbulence: High Plasma Beta Regime

Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers)

Investigating the IBEX Ribbon Structure a Solar Cycle Apart

Temperature of the Polar Inner Heliosheath: Connection to Solar Activity

Proton Equatorial Pitch Angle Distributions in Jupiter's Inner Magnetosphere

Relative In-flight Response of IBEX-Lo to Interstellar Neutral Helium Atoms

Collaborators (14)

Eberhard Moebius

Nicholas Sarlis

James Ryan

Joe Giacalone

G. P. Zank

Jamey R. Szalay

André Galli

Ratan Kumar Bera

Jacob Heerikhuisen

Paweł Swaczyna

Nikolai Pogorelov

Michael L. Stevens

Riddhi Bandyopadhyay

Ali Sulaiman

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