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).
| Keyword
| Occurrences
|
|---|
| Sun: Coronal Mass Ejections
| 19
|
| Solar Wind [H]
| 19
|
| Magnetohydrodynamical Simulations
| 9
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 7
|
| Physics - Space Physics [H]
| 7
|
| Space Weather
| 7
|
| Magnetohydrodynamics [S]
| 6
|
| Sun: Magnetic Fields
| 6
|
| Corotating Streams
| 5
|
| Sun: Corona [S]
| 5
|
| Methods: Numerical
| 3
|
| Driver Gases
| 3
|
| Sun: Heliosphere [H]
| 3
|
| Interplanetary Physics: Interplanetary Shocks
| 3
|
| Interplanetary Physics: Ejecta
| 3
|
| And Magnetic Clouds
| 3
|
| Interplanetary Physics: Coronal Mass Ejections (4305
| 3
|
| 7513)
| 3
|
| The Sun [S]
| 2
|
| 7836)
| 2
|
| Galactic Cosmic Rays
| 2
|
| Convolutional Neural Networks
| 2
|
| Magnetic Fields
| 2
|
| Interplanetary Physics: Mhd Waves And Turbulence (2752
| 2
|
| Interplanetary Physics [H]
| 2
|
| Mhd Simulation
| 2
|
| Solar Energetic Particle
| 1
|
| Solar Coronal Streamers
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Activity
| 1
|
| Self-consistent Structure
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Particle Acceleration
| 1
|
| Modeling
| 1
|
| Mars
| 1
|
| Magnetospheric Physics: Solar Wind/magnetosphere Interactions
| 1
|
| Magnetospheric Physics: Ring Current
| 1
|
| Magnetospheric Physics: Numerical Modeling
| 1
|
| Magnetospheric Physics: Magnetic Storms And Substorms (4305
| 1
|
| Magnetohydrodynamic (mhd)
| 1
|
| Magnetic Field
| 1
|
| Locally Divergence-free
| 1
|
| Kinematic Evolution
| 1
|
| Jupiter
| 1
|
| Juno
| 1
|
| Ionosphere: Particle Precipitation
| 1
|
| Interplanetary Transport
| 1
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 1
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 1
|
| Interplanetary Particle Acceleration [H]
| 1
|
| Interplanetary Coronal Mass Ejection
| 1
|
| Interaction
| 1
|
| Geomagnetic Storms
| 1
|
| Geomagnetic Storm
| 1
|
| Forecasting
| 1
|
| Flux Splitting
| 1
|
| Finite Volume Method
| 1
|
| Deflected Propagation
| 1
|
| Corotating Interaction Regions (cir)
| 1
|
| Computational Methods
| 1
|
| Basic Function
| 1
|
| Background Solar Wind
| 1
|
| Artificial Neural Network
| 1
|
| Artificial Compressibility
| 1
|
| Aneurysm
| 1
|
| Alfvén Waves
| 1
|
| 7954)
| 1
|
| Wls-eno
| 1
|
| Viscous Incompressible Flow
| 1
|
| Various Input
| 1
|
| Unstructured Grid
| 1
|
| Three-dimensional Mhd Simulation
| 1
|
| Super-elastic Collision
| 1
|
| Sun: Source Surface
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Interplanetary Scintillation
| 1
|
| Sun: Interaction
| 1
|
| Sun: Flares [S]
| 1
|
| Sun: Correlation
| 1
|
| Sun: Coronal Polarized Brightness Distribution
| 1
|
| Sun: Coronal Magnetic Field Distribution
| 1
|
| Sun: Collision Nature
| 1
|
| Sun: Cir
| 1
|
| 3200)
| 1
|
| Speed Prediction
| 1
|
| Space Weather: Models
| 1
|
| Space Plasma Physics: Mathematical And Numerical Techniques (0500
| 1
|
| Solar-terrestrial Relations
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Energetic Particles (sep)
| 1
|
| Sun: Artificial Neural Network Technique
| 1
|