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: 0.217 (must be ≥ 0.15 for author to be listed in HelioIndex)
Heliosphere fraction: 0.812 (H)
| Keyword
| Occurrences
|
|---|
| Solar Wind [H]
| 5
| | Sun: Heliosphere [H]
| 5
| | Jupiter
| 4
| | Simulation
| 3
| | Cosmic Rays
| 3
| | Magnetohydrodynamics [S]
| 3
| | Galactic Cosmic Rays
| 3
| | Inner Magnetosphere
| 3
| | Interchange Instability
| 3
| | Turbulence
| 2
| | Interplanetary Turbulence [H]
| 2
| | Pickup Ions
| 2
| | Injection
| 2
| | Magnetosphere-ionosphere Coupling
| 1
| | Magnetosphere-ionosphere
| 1
| | Magnetosphere
| 1
| | Magnetopause Reconnection
| 1
| | Lunar Surface
| 1
| | Ism: Magnetic Fields
| 1
| | Ionospheric Conductance
| 1
| | Interstellar Plasma
| 1
| | Interplanetary Shocks [H]
| 1
| | Hlld
| 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
| | Planetary Science
| 1
| | Planetary Magnetospheres
| 1
| | Numerical Simulation
| 1
| | Methods: Numerical
| 1
| | Main Auroral Oval
| 1
| | Magnetospheric Convection
| 1
| | Corotating Streams
| 1
| | Co-rotating Streams
| 1
| | Riemann Solver
| 1
|
Created on Wed Apr 8 05:01:04 2026.
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