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
|
|---|
| Magnetohydrodynamics [S]
| 39
|
| Sun: Corona [S]
| 24
|
| Solar Wind [H]
| 21
|
| Sun: Coronal Mass Ejections
| 19
|
| Methods: Numerical
| 11
|
| Magnetohydrodynamical Simulations
| 8
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 7
|
| Interplanetary Medium [H]
| 7
|
| Waves
| 4
|
| Space Weather
| 4
|
| Sun: Solar Wind [H]
| 3
|
| Sun: Magnetic Fields
| 3
|
| Physics - Space Physics [H]
| 3
|
| Sun: Atmosphere [S]
| 3
|
| Magnetohydrodynamic Waves
| 3
|
| Solar Cycle
| 3
|
| Sun: Heliosphere [H]
| 3
|
| Magnetic Fields
| 3
|
| Physics - Plasma Physics [H]
| 2
|
| Solar Physics [S]
| 2
|
| Magnetohydrodynamics And Plasmas
| 2
|
| Solar Coronal Waves [S]
| 2
|
| Solar Coronal Mass Ejection Shocks
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Astrophysics
| 2
|
| Sun: Magnetic Topology
| 2
|
| Sun: Interior [S]
| 2
|
| Alfven Waves
| 2
|
| Plasma Dynamics And Flow
| 2
|
| Tokamaks Spherical Tokamaks
| 2
|
| Sun: Active Regions
| 2
|
| Polarization Field.
| 1
|
| Plasma Diagnostic Techniques And Instrumentation
| 1
|
| Planet Hosting Stars
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Physics - Computational Physics
| 1
|
| Monte Carlo Methods
| 1
|
| Magnetogram
| 1
|
| Line: Profiles
| 1
|
| Jeans Instability
| 1
|
| Ism: Jets And Outflows
| 1
|
| Ionization
| 1
|
| Interplanetary Physics [H]
| 1
|
| Interplanetary Particle Acceleration [H]
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Inhomogeneous Plasma
| 1
|
| Hydrodynamics
| 1
|
| Hydrodynamical Simulations
| 1
|
| High Resolution Spectroscopy
| 1
|
| G Dwarf Stars
| 1
|
| Flux Emergence.
| 1
|
| Extreme Ultraviolet Astronomy
| 1
|
| Exoplanets
| 1
|
| Electron Impact Ionization
| 1
|
| Distributed Computing
| 1
|
| Cosmic Rays
| 1
|
| Computational Mhd
| 1
|
| CME Propagation
| 1
|
| Termination Shock
| 1
|
| Techniques: Spectroscopic
| 1
|
| Sun: UV Radiation [S]
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Sun: Structures
| 1
|
| Sun: Solar Cycle
| 1
|
| Sun: Photosphere [S]
| 1
|
| Sun: Observations
| 1
|
| Sun: Models
| 1
|
| Sun: Heliosheath
| 1
|
| Sun: Heliopause
| 1
|
| Sun: E
| 1
|
| Stellar Winds
| 1
|
| Stellar Coronae
| 1
|
| Spectrophotometry
| 1
|
| Space Plasmas [H]
| 1
|
| Space Plasma Physics
| 1
|
| Solar Wind CME Initiation
| 1
|
| Solar Transition Region
| 1
|
| Solar Spectral Irradiance
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Flares And CMEs
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Coronal Lines
| 1
|
| Slow Solar Wind [H]
| 1
|
| Shock Waves
| 1
|
| Scientific Computing
| 1
|
| Relativity
| 1
|
| Radiative Transfer [S]
| 1
|
| Quiet Sun
| 1
|
| Alfvén Waves
| 1
|
| Waves Oscillations And Instabilities In Plasmas And Intense Beams
| 1
|