Keyword data for ORCID ID 0000-0003-0541-0597
The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
Solar keyword fraction: 0.194 (must be ≥ 0.15 for author to be listed in HelioIndex)
Heliosphere fraction: 0.812 (H)
| Keyword
| Occurrences
|
|---|
| Sun: Heliosphere [H]
| 5
| | Solar Wind [H]
| 5
| | Jupiter
| 4
| | Inner Magnetosphere
| 3
| | Cosmic Rays
| 3
| | Simulation
| 3
| | Interchange Instability
| 3
| | Magnetohydrodynamics [S]
| 3
| | Galactic Cosmic Rays
| 3
| | Interplanetary Turbulence [H]
| 2
| | Injection
| 2
| | Pickup Ions
| 2
| | Turbulence
| 2
| | Magnetospheric Convection
| 1
| | Magnetosphere-ionosphere Coupling
| 1
| | Magnetosphere-ionosphere
| 1
| | Magnetosphere
| 1
| | Magnetosheath
| 1
| | Magnetopause Reconnection
| 1
| | Lunar Surface
| 1
| | Ism: Magnetic Fields
| 1
| | Ionospheric Conductance
| 1
| | Interstellar Plasma
| 1
| | Interplanetary Shocks [H]
| 1
| | Hlld
| 1
| | High-speed Jets
| 1
| | Foreshock Transients
| 1
| | Field-aligned Current
| 1
| | The Moon
| 1
| | Space Weather
| 1
| | Space Physics
| 1
| | Solar-planetary Interactions
| 1
| | Solar Wind-magnetosphere Coupling
| 1
| | Solar Wind Discontinuity
| 1
| | Agyrotropic Electron Distributions
| 1
| | Reconnection
| 1
| | Planetary Science
| 1
| | Planetary Magnetospheres
| 1
| | Numerical Simulation
| 1
| | Methods: Numerical
| 1
| | Main Auroral Oval
| 1
| | Corotating Streams
| 1
| | Co-rotating Streams
| 1
| | Bow Wave
| 1
| | Bow Shock
| 1
| | Riemann Solver
| 1
|
Created on Thu Oct 22 04:54:46 2026.
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