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
|
|---|
| Solar Wind [H]
| 23
|
| Sun: Coronal Mass Ejections
| 21
|
| Magnetohydrodynamical Simulations
| 11
|
| Space Weather
| 10
|
| Sun: Magnetic Fields
| 7
|
| Magnetohydrodynamics [S]
| 7
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 6
|
| Sun: Corona [S]
| 6
|
| Corotating Streams
| 5
|
| Physics - Space Physics [H]
| 5
|
| Sun: Heliosphere [H]
| 5
|
| And Magnetic Clouds
| 3
|
| Interplanetary Physics: Coronal Mass Ejections (4305
| 3
|
| Interplanetary Physics [H]
| 3
|
| Solar Coronal Mass Ejection Shocks
| 3
|
| Magnetic Fields
| 3
|
| Driver Gases
| 3
|
| 7513)
| 3
|
| Convolutional Neural Networks
| 3
|
| Interplanetary Physics: Interplanetary Shocks
| 3
|
| Methods: Numerical
| 3
|
| Interplanetary Physics: Ejecta
| 3
|
| Galactic Cosmic Rays
| 2
|
| Interplanetary Physics: Mhd Waves And Turbulence (2752
| 2
|
| The Sun [S]
| 2
|
| Solar Activity
| 2
|
| Mhd Simulation
| 2
|
| Solar Coronal Streamers
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Shock
| 1
|
| Pic Simulation
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Modeling
| 1
|
| Mms Observation
| 1
|
| Mars
| 1
|
| Magnetospheric Physics: Solar Wind/magnetosphere Interactions
| 1
|
| Magnetospheric Physics: Numerical Modeling
| 1
|
| Magnetospheric Physics: Magnetic Storms And Substorms (4305
| 1
|
| Magnetohydrodynamic (mhd)
| 1
|
| Magnetic Field
| 1
|
| Machine Learning
| 1
|
| Locally Divergence-free
| 1
|
| Kinematic Evolution
| 1
|
| Jupiter
| 1
|
| Juno
| 1
|
| Interplanetary Transport
| 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
|
| Core Field
| 1
|
| Computational Methods
| 1
|
| Basic Function
| 1
|
| Background Solar Wind
| 1
|
| Artificial Neural Network
| 1
|
| Artificial Compressibility
| 1
|
| Aneurysm
| 1
|
| Viscous Incompressible Flow
| 1
|
| Various Input
| 1
|
| Unstructured Grid
| 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
|
| Sun: Artificial Neural Network Technique
| 1
|
| Sun: Active Regions
| 1
|
| Speed Prediction
| 1
|
| Space Plasma Physics: Mathematical And Numerical Techniques (0500
| 1
|
| Solar-terrestrial Relations
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Energetic Particles (sep)
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Energetic Particle
| 1
|
| Solar E Corona
| 1
|
| Alfvén Waves
| 1
|
| Active Flux Rope
| 1
|
| 7954)
| 1
|
| 7836)
| 1
|
| Wls-eno
| 1
|