JH
0000-0001-8179-417X Employment
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Publications (141)
- Ground Calibration of the Helios ENA Rapid MApper (HERMA) for Heliospheric Boundary Exploration Save
- A Nonspherical Source Surface Model for the Solar Coronal Magnetic Field Save
- Energy Redistribution of Ion-scale Turbulence from Quasi-perpendicular to Quasi-parallel Wavevectors as Induced by Field-particle Interactions Save
- Optimization Algorithm for Determining the Source Surface Radius Based on Parker Solar Probe In Situ Measurements From Encounters 1 to 19 Save
- Non-adiabatic entropy increase in the solar wind governed by velocity spikes Save
- Alpha-particle Heating and Anisotropy in Solar Wind Turbulence: Insights from Parker Solar Probe Observations and Particle-in-cell Simulations Save
- Imaging Magnetically Driven Astrospheres: A Forward Modeling Approach Save
- Flapping of Multifold Heliospheric Current Sheet Observed by Parker Solar Probe Save
- Generation of Proton Beams at Switchback Boundary-like Rotational Discontinuities in the Solar Wind Save
- Influence of Solar Polar Magnetic Fields on the Propagation of Coronal Mass Ejections Save
- Ion Stochastic Heating by Wave-induced Field Line Curvature in Space Plasmas Save
- Chaotic Motion of Ions in Finite-amplitude Low-frequency Alfvén Waves Save
- Distinct Source Regions for Slow Solar Wind Populations Differentiated by Residual Energy during Parker Solar Probe Encounter 7 Save
- Multiscale Magnetic Reconnection in the Genesis of Young Slow Solar Wind Save
- Spectral Evolution of Pickup Ions across Interplanetary Shocks in the Outer Heliosphere: Observational Constraints and Transport Simulations Save
- Unveiling the Global Characteristics of Turbulence in the Venusian Space Environment Save
- Nonstandard Collapse of Strong Langmuir Turbulence: Constraints on Its Occurrence and Observation in the Solar Corona Save
- Statistics of the Interplanetary Magnetic Field from 0.1 to 30 au. II. Dynamical Variability Save
- Spectral Features of the Energy-containing Range and the Inertial Range in Fast Solar Wind Turbulence Save
- Fine-scale activity driven by magnetic reconnection within coronal microjets Save