Stuart Bale

Professor of Physics

University of California, Berkeley

United States

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About

Stuart Bale is a Professor of Physics at the University of California Berkeley, USA. His research focuses on plasma physics, particularly in the context of solar phenomena, magnetic reconnection, and the behavior of energetic particles. His recent publications include studies on solar radio bursts, whistler wave polarization, and observations from the Parker Solar Probe, highlighting his contributions to understanding complex astrophysical processes.

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Collaborators (22)

Kristopher Klein

Associate Professor

University of Arizona

UNITED STATES

Stuart Bale

Research Interests

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About

Articles (30)

Large-amplitude Whistler Precursors and >MeV Particles Observed at a Weak Interplanetary Shock by Parker Solar Probe

Generalized Two Thermal Regime Approach: Bipoly Fluid Modeling

Polarization Properties of Whistler Waves From the First 17 Parker Solar Probe Encounters

Plasma Instability in Front of Ejected Energetic Electrons and Type III Solar Radio Bursts

Calibration of Electrically Short Antennas Using the l = 2 Spherical Harmonic Expansion Coefficients of the Radio Brightness Distribution on the Sky Between 0.5 and 6.8 MHz

Formation of magnetic switchbacks via expanding Alfvén waves

Highly Polarized Type III Storm Observed with Parker Solar Probe

Parker Solar Probe Observations of a Highly Energetic and Asymmetric Reconnecting Heliospheric Current Sheet during Encounter 13

Magnetic Reconnection–driven Energization of Protons up to ∼400 keV at the Near-Sun Heliospheric Current Sheet

Impulsive Solar Flares in the Parker Solar Probe Era. I. Low-energy Electron, Proton, and Alpha Beams

Embedded Coherent Structures from Magnetohydrodynamics to Sub-ion Scales in Turbulent Solar Wind at 0.17 au

Radial Variations in Solar Type III Radio Bursts

Extended Cyclotron Resonant Heating of the Turbulent Solar Wind

Near Subsonic Solar Wind Outflow from an Active Region

Coexistence of Antisunward and Sunward Ion Cyclotron Waves in the Near-Sun Solar Wind: Excitation by the Proton Cyclotron Instability

Multiple Subscale Magnetic Reconnection Embedded inside a Heliospheric Current Sheet Reconnection Exhaust: Evidence for Flux Rope Merging

Compositional Metrics of Fast and Slow Alfvénic Solar Wind Emerging from Coronal Holes and Their Boundaries

Parker Solar Probe Observations of Energetic Particles in the Flank of a Coronal Mass Ejection Close to the Sun

Resonance of Low-frequency Electromagnetic and Ion-sound Modes in the Solar Wind

Evolution of Electron Acceleration by Corotating Interaction Region Shocks at 1 au

Switchbacks, microstreams, and broadband turbulence in the solar wind

Quantifying the Energy Budget in the Solar Wind from 13.3 to 100 Solar Radii

Reconstruction of polarization properties of whistler waves from two magnetic and two electric field components: Application to Parker Solar Probe measurements

Interchange reconnection as the source of the fast solar wind within coronal holes

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

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

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

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

The Radial Distribution of Ion-scale Waves in the Inner Heliosphere

A Dust Detection Database for the Inner Heliosphere Using the Parker Solar Probe Spacecraft

Collaborators (22)

Kristopher Klein

Romain Meyrand

Thierry Dudok de Wit

Frantisek Nemec

Francesco Pecora

Lorenzo Matteini

Milan Maksimovic

Ondrej Santolik

W. S. Kurth

Adam Szabo

Jamey R. Szalay

Jasper Halekas

Athanasios Kouloumvakos

Chen Shi

Matthieu Kretzschmar

David M. Malaspina

Michael Swisdak

Liu Yang

Michael McManus

Susan Lepri

Alfred Mallet

Michael L. Stevens

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