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]
| 56
|
| Physics - Space Physics [H]
| 30
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 30
|
| Turbulence
| 26
|
| Interplanetary Turbulence [H]
| 26
|
| Physics - Plasma Physics [H]
| 18
|
| Space Plasmas [H]
| 14
|
| Sun: Heliosphere [H]
| 12
|
| Waves
| 12
|
| Plasmas
| 11
|
| Magnetohydrodynamics [S]
| 10
|
| Alfven Waves
| 10
|
| Magnetic Fields
| 9
|
| Solar Magnetic Reconnection
| 9
|
| Sun: Coronal Mass Ejections
| 7
|
| Sun: Corona [S]
| 6
|
| Magnetic Reconnection
| 6
|
| Methods: Numerical
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Sun: Transition Region [S]
| 5
|
| Sun: Uv Radiation [S]
| 4
|
| Acceleration Of Particles
| 4
|
| Shock Waves
| 4
|
| Astrophysics - Earth And Planetary Astrophysics
| 4
|
| Planetary Magnetospheres
| 4
|
| Slow Solar Wind [H]
| 4
|
| Interplanetary Magnetic Fields [H]
| 4
|
| Planets And Satellites: Magnetic Fields
| 3
|
| Sunspots [S]
| 3
|
| Planetary Bow Shocks
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Sun: Oscillations [S]
| 3
|
| Techniques: Spectroscopic
| 2
|
| Sun: Magnetic Fields
| 2
|
| Sun: Filaments [S]
| 2
|
| Solar-planetary Interactions
| 2
|
| Solar Physics [S]
| 2
|
| Solar Activity
| 2
|
| Mercury (planet)
| 2
|
| Magnetohydrodynamical Simulations
| 2
|
| Line: Profiles
| 2
|
| Alfvén Waves
| 2
|
| Sun: Photosphere [S]
| 2
|
| Solar Particle Emission
| 1
|
| Tangential Discontinuity
| 1
|
| Solar Active Regions [S]
| 1
|
| Small Flux Rope
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Shocks
| 1
|
| Solar Wind Speed
| 1
|
| Rolling Back Magnetic Field Lines
| 1
|
| Red Equatorial Aurora
| 1
|
| Quiet Sun
| 1
|
| Potential Field Source Surface
| 1
|
| Solar-terrestrial Relations
| 1
|
| Plasma Physics
| 1
|
| Plasma Astrophysics
| 1
|
| Planets And Satellites: Terrestrial Planets
| 1
|
| Planets And Satellites: Physical Evolution
| 1
|
| Sun: Abundances
| 1
|
| Planetary Science
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Coronal
| 1
|
| Planetary Boundary Layers
| 1
|
| Sun: Coronal Mass Ejection: Cmes
| 1
|
| Sun: Granulation [S]
| 1
|
| Physics - Geophysics
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Parallel Electric Field
| 1
|
| Sun: Heating
| 1
|
| The Sun [S]
| 1
|
| Maunder Minimum
| 1
|
| Mars
| 1
|
| Sun: Low Coronal Signatures
| 1
|
| Asteroids
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Whistler Wave
| 1
|
| Sun: Turbulence
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Physics [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| Supergranulation
| 1
|
| Interplanetary Dust
| 1
|
| Interplanetary Discontinuities
| 1
|
| Interchange Reconnection
| 1
|
| Geomagnetic Activity
| 1
|
| Fast Solar Wind
| 1
|
| Energy Dissipation
| 1
|
| Electron Acceleration
| 1
|
| Earth
| 1
|
| Convolutional Neural Network
| 1
|
| Computational Methods
| 1
|
| Comet Tails
| 1
|
| Collisionless Shock
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Dynamo
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Atmosphere
| 1
|