BV
Bart van der Holst
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
0000-0001-5260-3944
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Publications (123)
- Modulation of Galactic Cosmic Rays in Corotating Interaction Regions: Diffusion Dominates over Drifts and Advection Save
- Global Multi-ion Solar Wind Model. I. Ion Temperatures Save
- Dynamics of the Upwind Heliosphere Due to Data-driven Solar Wind and Magnetic Field Variations and Implications for Wave Propagation into the Very Local Interstellar Medium Save
- Pickup Ion Production and Turbulence in the Global Heliosphere Save
- Evolution of Coronal Mass Ejections in Different Data-driven Solar Wind Conditions Save
- Modeling the Energy Release in Solar Eruptive Events Save
- High-resolution Simulation of Coronal Mass Ejection–Corotating Interaction Region Interactions: Mesoscale Solar Wind Structure Formation Observable by the SWIFT Constellation Save
- Validation of Long-term Solar Coronal Modeling Using FORWARD Save
- Consequences of Hot Electrons for the Structure of the Outer Heliosphere Save
- Erratum: “Solar Wind Driven from GONG Magnetograms in the Last Solar Cycle” (2024, ApJ, 965, 1) Save
- Erratum: “Modeling the Solar Wind during Different Phases of the Last Solar Cycle” (2023, ApJL, 946, L47) Save
- Evolution of Coronal Mass Ejections in the Solar Wind using Data-Driven Numerical Models Save
- AWSoM solar wind model with charge states and ion temperatures Save
- Determining the CME Onset Mechanism Save
- Global Modeling of Heavy Ions in the Solar Corona and Inner Heliosphere with Multi-Ion-AWSoM Save
- Studying the Long-Term Variability of the Solar Corona Using Modeling and Remote-Sensing Observations Save
- Sun-to-Earth CME Modeling with Data Assimilation and Uncertainty Quantification Save
- The solar wind in the last solar cycle driven by ADAPT-GONG and GONG magnetograms Save
- Unified Alfven Wave Turbulence Based Model for Energy and Particle Transport in Solar Corona and Heliosphere Save
- Decent Estimate of CME Arrival time from a Data-assimilated Ensemble in the Alfvén Wave Solar atmosphere Model (DECADE-AWSoM) Save